diff --git a/.gitignore b/.gitignore new file mode 100644 index 00000000..e69de29b diff --git a/CLAUDE.md b/CLAUDE.md new file mode 100644 index 00000000..628204eb --- /dev/null +++ b/CLAUDE.md @@ -0,0 +1,39 @@ +# CLAUDE.md + +This file provides guidance to Claude Code (claude.ai/code) when working with code in this repository. + +## Repository overview + +Static website for the PhotoDissociation Region Toolbox (dustem.astro.umd.edu), served via Apache SSI (Server Side Includes — ``). Describes PDR modeling, hosts model images/FITS files, and documents the `pdrtpy` Python package (https://pdrtpy.readthedocs.io). There is no build step, bundler, or JS framework for the static pages — HTML is either hand-edited or generated by the Python script in `autogen/`. + +## Regenerating the model pages + +The `models/` directory (one subdirectory per ModelSet, e.g. `wk2006_Z1.0_constant_density`, `smc_Z0.2_L45_constant_density`) is generated output, not hand-edited. Each ModelSet directory contains generated `.fits`, `.png`, and `.html` files for every model ratio/quantity, plus an `index.html`. + +To regenerate: + +``` +cd autogen +python make_model_webpages.py # generate all non-KOSMA-tau ModelSets +python make_model_webpages.py -k # also include KOSMA-tau (kt*) models +python make_model_webpages.py -m # only a given modelset +python make_model_webpages.py -q # quick: skip plot generation, only rebuild all_models index +``` + +This requires `pdrtpy` installed (`ModelSet`, `ModelPlot` from `pdrtpy.modelset` / `pdrtpy.plot.modelplot`) and writes output to `../models.new/` (a sibling directory, NOT `../models/` — output must be reviewed and manually promoted/renamed into `models/` before it takes effect on the site). The script pools across `os.cpu_count() - 2` processes via `multiprocessing.Pool`. + +Key behaviors to know when touching `autogen/make_model_webpages.py`: + +- `lmc` and `wk2006` model name prefixes are currently skipped entirely (line ~65), as is any `kt*` set when `-k`/`--kosmatau` is not passed. +- Per-ModelSet HTML "explain" text and display titles are hardcoded in `explain` and `model_title` dicts inside `process_modelset()` — add entries there when introducing a new ModelSet family (matched by prefix of `ms.keyname`). +- Model titles/units arrive from `pdrtpy` containing LaTeX (`$...$`); the script does manual `.replace()` cleanup to turn them into HTML/entities before rendering. If `$` still appears in a title after cleanup, the script prints `############ OOPS missed some latex ...` — check for this in output when adding new model quantities. +- Ionized-gas line-ratio models (`model.wcs.wcs.ctype[0] == "T_e"`) are plotted/labeled differently (electron temperature/density axes) than standard PDR density/FUV-flux models — this drives `ms.keyname = "hii"` and different axis labels. +- Each ModelSet directory also gets a `_models.tgz` tarball referenced from its page; this is not created by the script and must exist separately in `models/`. It is not tracked by github since it is a large binary file. Marc ensures these files are up to date. + +Jinja2 templates live in `autogen/`: `index_page_jinja_template.html` (per-ModelSet index), `model_page_jinja_template.html` (per-model-quantity page), `all_models_page_jinja_template.html` (top-level `models/index.html` listing all ModelSets). These duplicate the nav/head markup rather than sharing it with the hand-written pages — when nav changes, update it in the templates *and* in every top-level `.html` file and `includes/nav.inc`. + +## Page structure conventions + +- `includes/head.inc`, `includes/nav.inc`, `includes/footer.inc` are SSI includes intended to be shared across hand-written pages, but note the top-level pages (`index.html`, `models.html`, `tools.html`, `docs.html`) inline their own copy of the nav markup rather than including `nav.inc` — check which pattern a given page already uses before editing. +- CSS: `css/pdrt.css` is site-specific; `freelancer/css/*` is the vendored Start Bootstrap "Freelancer" theme (https://startbootstrap.com/themes/freelancer/) — don't hand-edit vendored files, override in `pdrt.css` instead. +- Root-relative paths (`/css/...`, `/includes/...`, `/models/...`) are used throughout — pages assume they are served from the site root, not from a subdirectory. diff --git a/autogen/all_models_page_jinja_template.html b/autogen/all_models_page_jinja_template.html index 664e3de2..d7053047 100755 --- a/autogen/all_models_page_jinja_template.html +++ b/autogen/all_models_page_jinja_template.html @@ -35,7 +35,8 @@

Links to All Available ModelSets

-Click on the description to explore a ModelSet (see plots, download FITS files). +To see plots and download individual FITS files for a given ModelSet, click on its ModelSet Description. + {% for key,value in all_models.items() %} diff --git a/autogen/index_page_jinja_template.html b/autogen/index_page_jinja_template.html index 14fc54d9..b315acd0 100755 --- a/autogen/index_page_jinja_template.html +++ b/autogen/index_page_jinja_template.html @@ -36,7 +36,7 @@

{{modelset.header}}

Below are links to the individual FITS files -and plots in the {{modelset.name}} {{modelset.name}} z={{modelset.z}} losangle={{modelset.losangle}} ModelSet. We also provide a gzipped tarball of all the {{modelset.keyname}} FITS and PNG files.

ModelSet name in pdrtpyModelSet Description
diff --git a/autogen/make_model_webpages.py b/autogen/make_model_webpages.py index c1777635..7dca7afa 100755 --- a/autogen/make_model_webpages.py +++ b/autogen/make_model_webpages.py @@ -6,21 +6,104 @@ import os import jinja2 import argparse +import sys +import warnings +from pathlib import Path +warnings.simplefilter("ignore",SyntaxWarning) +EXPLAIN = dict() +EXPLAIN["lmc"] = 'The models in the wk2006 Large Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers.' +EXPLAIN["smc"] = 'The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers.' +EXPLAIN["wk2006"] = 'The models in the wk2006 ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers.' +EXPLAIN["wk2020"] = 'The models in the wk2020 ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use these parameters. More details are in the FITS headers.' +EXPLAIN["kt2013"] = 'The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.' +EXPLAIN["kt2020"] = 'The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.' +EXPLAIN["hii"] = 'We assume that the line emission is in the optically thin limit so that the ratio of emissivities is given by the ratio of volume emissivity. For \({\\rm Ar^{+2}}\) , and \({\\rm Ar^{+4}}\) , we use CHIANTI ( Dere et al (1997); DelZanna et al. (2022)) using the default values for the A values and collision strengths. For \({\\rm Fe^+}\) we substituted the default values in CHIANTI with Einstein A values from Deb & Hibbert (2011) and collision strengths from Smyth et al. (2019) . The emissivity ratios are found in the temperature range from \(T_e=10^3\) K to \(10^4\) K, and the density range from \(n_e = 10^2~{\\rm cm^{-3}}\) to \(10^6~{\\rm cm^{-3}}\). ' -def init_processes(l): - global lock - lock = l +def skip_modelset(n, kosmatau): + """Determine whether a ModelSet should be excluded from generation. + + KOSMA-tau (``kt*``) sets are only included when explicitly requested; + ``lmc`` and ``wk2006`` sets are always skipped (see module docstring + in ``process_modelset``. KT is typically skipped because we don't + expect an update for these models anytime soon. LMC and 2006 are skipped because + they are also static. They will be replaced/deprecated soon at which time the + second startswith should be removed. Or we make a generic --skip option which + defaults to kt* + + + Parameters + ---------- + n : str + ModelSet name, e.g. ``"wk2020"``, ``"smc"``, ``"kt2013wd01-7"``. + kosmatau : bool + If `True`, KOSMA-tau (``kt*``) ModelSets are allowed through. + + Returns + ------- + bool + `True` if the ModelSet named `n` should be skipped, `False` + otherwise. + """ + if n.startswith("kt") and not kosmatau: + print(f"skipping {n}") + return True + if n.startswith("lmc") or n.startswith("wk2006"): + print(f"skipping {n}") + return True + return False + class Page(): - def __init__(self, kosmatau): + """Generate the model webpages (per-ModelSet index pages, per-ratio + model pages, and the top-level all-models index page) into + ``../models.new``. + + Parameters + ---------- + kosmatau : bool + If `True`, include KOSMA-tau (``kt*``) ModelSets in addition to the + Wolfire/Kaufman and SMC ModelSets. + modelset : str, optional + If given, restrict generation to the ModelSet(s) with this name + (matches the ``name`` column of `ModelSet.all_sets()`, so e.g. a + KOSMA-tau name can still expand to multiple mass/medium variants). + Default is `None`, which processes all available ModelSets. + """ + + def __init__(self, kosmatau, modelset=None): self.env=jinja2.Environment(loader=jinja2.FileSystemLoader(".")) - self.base_dir = "../models.new" + self.base_dir = Path("../models.new") self.kosmatau = kosmatau + self.modelset = modelset + self.base_dir.mkdir(exist_ok=True) + # per-worker-process cache of (ModelSet,ModelPlot), populated lazily + # in process_ratio() so consecutive ratio tasks for the same + # ModelSet landing on the same forked worker skip re-loading the + # FITS tables. + self._ms_cache = dict() def write_all_models_page(self,all_models,all_names): - # don't instantiate these in __init__ or you get a + """Render and write the top-level ``models.new/index.html`` page + listing every generated ModelSet. + + Parameters + ---------- + all_models : dict + Mapping of ModelSet output directory name (`ms.dir`) to its + HTML-escaped description (`ms.header`), as populated by + `register_modelset`. + all_names : dict + Mapping of ModelSet output directory name (`ms.dir`) to its + `pdrtpy` ModelSet name (e.g. ``"wk2020"``), as populated by + `register_modelset`. + + Returns + ------- + None + """ + # don't instantiate these in __init__ or you get a # "TypeError: cannot pickle weakref" from Pool.starmap self.allmodelstemplatefile = 'all_models_page_jinja_template.html' self.allmodelstemplate = self.env.get_template(self.allmodelstemplatefile) @@ -29,60 +112,84 @@ def write_all_models_page(self,all_models,all_names): names = dict(reversed(sorted(list(all_names.items())))) #for key,value in wkfirst.items(): # print(key) + print("rendering all models...") output=self.allmodelstemplate.render(all_models=wkfirst,all_names=names) fh = open(f'{self.base_dir}/index.html','w') fh.write(output) fh.close() - def make_page(self,all_models,all_names,lock,quick=False): - # check all models.tab files and existence of all therein + def selected_modelsets(self): + """Look up and filter the ModelSet specs to generate. + + Starts from `ModelSet.all_sets()`, restricts to `self.modelset` + if one was given, normalizes masked ``mass`` values to `None` + (masked values are not hashable and are used as part of a cache + key in `process_ratio`), and drops any ModelSet excluded by + `skip_modelset`. + + Returns + ------- + list of tuple + Each tuple is ``(n, z, losangle, md, m)`` where: + + n : str + ModelSet name. + z : float + Metallicity relative to solar. + losangle : float + Line-of-sight viewing angle in degrees (``0`` = face-on). + md : str + Medium type, e.g. ``"constant density"``, ``"clumpy"``, + ``"non-clumpy"``. + m : float or None + Clump mass in solar masses, or `None` for ModelSets that + don't have a mass axis. + """ t = ModelSet.all_sets() - ziplist = zip(list(t["name"]),list(t["z"]),list(t['losangle']),list(t["medium"]),list(t["mass"])) - - if False: - print("single threading...") - for name,metallicity,losangle,medium,mass in ziplist: - self.process_modelset(name,metallicity,losangle,medium,mass) - else: - print("pooling...") - pool = Pool(os.cpu_count()-2,initializer=init_processes,initargs=(lock,)) - pool.starmap(self.process_modelset,ziplist) - - def process_modelset(self,n,z,losangle,md,m): - #debug = True - #if debug and "lmc" not in n: return - if n.startswith("kt") and not self.kosmatau: - print(f"skipping {n}") - return - if n.startswith("lmc") or n.startswith("smc") or n.startswith("wk2006"): - print(f"skipping {n}") - return - print(f'Making page for {n,z,losangle,md,m}') - explain = dict() - explain["lmc"] = 'The models in the wk2006 Large Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers.' - explain["smc"] = 'The models in the wk2006 Small Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers.' - explain["wk2006"] = 'The models in the wk2006 ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers.' - explain["wk2020"] = 'The models in the wk2020 ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use these parameters. More details are in the FITS headers.' - explain["kt2013"] = 'The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.' - explain["kt2020"] = 'The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.' - explain["hii"] = 'We assume that the line emission is in the optically thin limit so that the ratio of emissivities is given by the ratio of volume emissivity. For \({\\rm Ar^{+2}}\) , and \({\\rm Ar^{+4}}\) , we use CHIANTI ( Dere et al (1997); DelZanna et al. (2022)) using the default values for the A values and collision strengths. For \({\\rm Fe^+}\) we substituted the default values in CHIANTI with Einstein A values from Deb & Hibbert (2011) and collision strengths from Smyth et al. (2019) . The emissivity ratios are found in the temperature range from \(T_e=10^3\) K to \(10^4\) K, and the density range from \(n_e = 10^2~{\\rm cm^{-3}}\) to \(10^6~{\\rm cm^{-3}}\). ' - model_title = dict() - model_title["wk2006"] = "Wolfire/Kaufman 2006" - model_title["smc"] = "Wolfire/Kaufman 2006 Small Magellanic Cloud " - model_title["lmc"] = "Wolfire/Kaufman 2006 Large Magellanic Cloud" - model_title["wk2020"] = "Wolfire/Kaufman 2020" - model_title["kt2013"] = "KOSMA-tau 2013" - model_title["kt2020"] = "KOSMA-tau 2020" - - success = True - failed = list() - pagetemplatefile = 'model_page_jinja_template.html' - pagetemplate = self.env.get_template(pagetemplatefile) - indextemplatefile = 'index_page_jinja_template.html' - indextemplate = self.env.get_template(indextemplatefile) + if self.modelset is not None: + t = t[t["name"] == self.modelset] + if len(t) == 0: + print(f"no ModelSet found matching name '{self.modelset}'") + return [] + ziplist = list(zip(list(t["name"]),list(t["z"]),list(t['losangle']),list(t["medium"]),list(t["mass"]))) + # normalize masked mass values to None so they're hashable (used as + # part of the per-worker ModelSet cache key in process_ratio) + ziplist = [(n,z,losangle,md,None if ma.is_masked(m) else m) for n,z,losangle,md,m in ziplist] + return [spec for spec in ziplist if not skip_modelset(spec[0], self.kosmatau)] - ms = ModelSet(name=n,z=z,losangle=losangle,medium=md,mass=m) + def register_modelset(self,n,z,losangle,md,m,all_models,all_names): + """Build a `ModelSet` and register it in `all_models`/`all_names`. + + Cheap (no plotting) -- safe to run serially in the main process. + Parameters + ---------- + n : str + ModelSet name. + z : float + Metallicity relative to solar. + losangle : float + Line-of-sight viewing angle in degrees (``0`` = face-on). + md : str + Medium type, e.g. ``"constant density"``, ``"clumpy"``, + ``"non-clumpy"``. + m : float or None + Clump mass in solar masses, or `None` for ModelSets that + don't have a mass axis. + all_models : dict + Mapping of ModelSet output directory name to HTML-escaped + description; updated in place with this ModelSet's entry. + all_names : dict + Mapping of ModelSet output directory name to `pdrtpy` + ModelSet name; updated in place with this ModelSet's entry. + + Returns + ------- + pdrtpy.modelset.ModelSet + The constructed ModelSet, with `dir`, `header`, `keyname`, and + `tarball` attributes attached for use by the caller. + """ + ms = ModelSet(name=n,z=z,losangle=losangle,medium=md,mass=m) if n.startswith("kt2013"): ms.keyname = "kt2013" else: @@ -95,121 +202,241 @@ def process_modelset(self,n,z,losangle,md,m): # KT models don't have losangle ms.dir = f'{n}_Z{z}_{md}_M{m}' ms.dir = ms.dir.replace(' ','_') - with lock: - all_models[ms.dir] = ms.header - all_names[ms.dir] = n - if quick: + all_models[ms.dir] = ms.header + all_names[ms.dir] = n + return ms + + def make_page(self,all_models,all_names,quick=False,jobs=None): + """Generate model webpages for every selected ModelSet. + + Registers all selected ModelSets serially, then (unless `quick`) + flattens every ModelSet's ratios into a single flat task list and + farms them out to a `multiprocessing.Pool` via `process_ratio`, + so parallelism is per-ratio rather than per-ModelSet. Results are + then grouped back by ModelSet directory to render each + ModelSet's ``index.html``. + + Parameters + ---------- + all_models : dict + Mapping of ModelSet output directory name to HTML-escaped + description; updated in place as ModelSets are registered. + all_names : dict + Mapping of ModelSet output directory name to `pdrtpy` + ModelSet name; updated in place as ModelSets are registered. + quick : bool, optional + If `True`, only register ModelSets (populate `all_models`/ + `all_names`) without generating any plots, FITS files, or + per-ratio/index HTML pages. Default is `False`. + jobs : int, optional + Number of worker processes to use for plotting. Default is + `None`, which uses `os.cpu_count()`. + + Returns + ------- + None + """ + specs = self.selected_modelsets() + + if quick: + # registration only, no plotting - not worth spinning up a Pool + for n,z,losangle,md,m in specs: + self.register_modelset(n,z,losangle,md,m,all_models,all_names) return - os.mkdir(f'{self.base_dir}/{ms.dir}') - mp = ModelPlot(ms) - # stop complaining about too many figures - mp._plt.rcParams.update({'figure.max_open_warning': 0}) - - i = 0 - numcols = 4 - table_contents = "" - for r in ms.table["ratio"]: - if i !=0 and i%numcols == 0: - table_contents+="\n" - try: - #ugly hack - modelfile = ms.table.loc[r]["filename"] - #print(modelfile) - if modelfile == "FEII25p99.fits": - model=ms.get_model(r,unit="erg/(cm3 s ion)") + ms_by_dir = dict() + tasks = list() + for n,z,losangle,md,m in specs: + print(f'Making page for {n,z,losangle,md,m}') + ms = self.register_modelset(n,z,losangle,md,m,all_models,all_names) + ms_by_dir[ms.dir] = ms + os.mkdir(f'{self.base_dir}/{ms.dir}') + for r in ms.table["ratio"]: + tasks.append((ms.dir,n,z,losangle,md,m,r)) + + if jobs is None: + jobs = os.cpu_count() + print(f"pooling {len(tasks)} ratio tasks with jobs={jobs}") + pool = Pool(jobs) + results = pool.starmap(self.process_ratio,tasks) + pool.close() + pool.join() + + by_dir = dict() + for ms_dir,success,table_cell,error in results: + by_dir.setdefault(ms_dir,list()).append((success,table_cell,error)) + + indextemplatefile = 'index_page_jinja_template.html' + indextemplate = self.env.get_template(indextemplatefile) + for ms_dir,ms in ms_by_dir.items(): + i = 0 + numcols = 4 + table_contents = "" + failed = list() + for success,table_cell,error in by_dir.get(ms_dir,[]): + if success: + if i !=0 and i%numcols == 0: + table_contents+="\n" + table_contents += table_cell + i = i+1 else: - model=ms.get_model(r) - if "/" in model._title: - #kluge for HII diagnotic files - if "FE" in modelfile or "AR" in modelfile: - model._title += " Emissivity Ratio" + failed.append(error) + if failed: + print("Couldn't open these models:",failed) + table_contents += '' + output=indextemplate.render(modelset=ms, + table_contents=table_contents) + fh = open(f'{self.base_dir}/{ms_dir}/index.html','w') + fh.write(output) + fh.close() + + def process_ratio(self,ms_dir,n,z,losangle,md,m,r): + """Plot and write out a single model ratio. + + Runs in a worker process. Rebuilds (or reuses, via + `self._ms_cache`) the `ModelSet`/`ModelPlot` for + ``(n, z, losangle, md, m)`` and generates the ratio's PNG plot, + FITS file, and per-ratio HTML page. + + Parameters + ---------- + ms_dir : str + Output directory name for this ratio's ModelSet (`ms.dir`, + as computed by `register_modelset`). + n : str + ModelSet name. + z : float + Metallicity relative to solar + losangle : float + Line-of-sight viewing angle in degrees (``0`` = face-on). + md : str + Medium type, e.g. ``"constant density"``, ``"clumpy"``, + ``"non-clumpy"``. + m : float or None + Clump mass in solar masses, or `None` for ModelSets that + don't have a mass axis. + r : str + Ratio identifier as found in `ms.table["ratio"]`, e.g. "CO76_CO10". + + Returns + ------- + tuple + ``(ms_dir, success, table_cell, error)`` where: + + ms_dir : str + Same as the `ms_dir` parameter, echoed back so results + from multiple workers can be regrouped by ModelSet. + success : bool + Whether the ratio was processed without error. + table_cell : str or None + HTML ``' + if model.wcs.wcs.ctype[0] == "T_e": + # Iron line ratios are function of electron temperature and electron density + # not H2 density and radiation field. + mp.plot(r,label=True,legend=False, + norm="zscale",cmap='plasma',aspect='auto') + keyname = "hii" + model.xaxis = "electron gas temperature Te" + model.yaxis = "electron density ne" + model.where = "from the ionized gas layer " + model.viewingangle="" + else: + mp.plot(r,yaxis_unit="Habing",label=True, legend=False, + norm="zscale",cmap='plasma') + keyname = ms.keyname + model.where = "from the surface " + model.xaxis = "cloud density n" + model.yaxis = "the FUV flux incident on the cloud G0" + if ms.name=="wk2020" or ms.name=="smc": + model.viewingangle=f"The above model is at a viewing angle of i={losangle} degrees, where i=0 is face-on." else: - if "FIR" not in model._title and "Surface" not in model._title and "A_V" not in model._title: - #kluge for HII diagnotic files - if "FE" in modelfile or "AR" in modelfile: - model._title += " Emissivity" - else: - model._title += " Intensity" - model._title = model._title.replace("$ \mu","$\mu") - model._title = model._title.replace("$\mu$","µ").replace("$_{FIR}$","FIR").replace("$_2$","2").replace("$A_V$","AV").replace("$^{13}$","13").replace("$A_V=0.01$","AV = 0.01") - #.replace("$T_S$","TS") - #print(f"doing {r} = {modelfile} , {modelfile}.png , title={model._title} CTYPE=[{model.wcs.wcs.ctype[0]},{model.wcs.wcs.ctype[1]}]") - if "$" in model._title: - print(f"############ OOPS missed some latex {model._title}") - fig_out = f'{ms.dir}/{modelfile}.png' - fig_html = f'{ms.dir}/{modelfile}.html' - fits_out = f'{ms.dir}/{modelfile}.fits' - f_html = f'{modelfile}.html' - table_contents += f'' - i = i+1 - if model.wcs.wcs.ctype[0] == "T_e": - # Iron line ratios are function of electron temperature and electron density - # not H2 density and radiation field. - mp.plot(r,label=True,legend=False, - norm="zscale",cmap='plasma',aspect='auto') - ms.keyname = "hii" - model.xaxis = "electron gas temperature Te" - model.yaxis = "electron density ne" - model.where = "from the ionized gas layer " model.viewingangle="" - else: - mp.plot(r,yaxis_unit="Habing",label=True, legend=False, - norm="zscale",cmap='plasma') - model.where = "from the surface " - model.xaxis = "cloud density n" - model.yaxis = "the FUV flux incident on the cloud G0" - if ms.name=="wk2020": - model.viewingangle=f"The above model is at a viewing angle of i={losangle} degrees, where i=0 is face-on." - else: - model.viewingangle="" - mp.savefig(f'{self.base_dir}/{fig_out}') - model.write(f'{self.base_dir}/{fits_out}') - # This is supposed to stop complaints about - # too many figures, but actually does not! - mp._plt.close(mp.figure) - output=pagetemplate.render(model=model,name=ms.name, - fitsfilename=f'{modelfile}.fits', - model_explain=explain[ms.keyname], - modelfile=modelfile) - fh = open(f'{self.base_dir}/{fig_html}','w') - fh.write(output) - #print(f'{self.base_dir}/{fig_html}') - # print(output) - # print("===========================================") - fh.close() - - except FileNotFoundError as fne: - print(fne) - success = False - failed.append(f'{r} {modelfile} : {str(fne)}\n') - except Exception as exc: - print(exc) - success = False - failed.append(f'{r} {modelfile} : {str(exc)}\n') - if not success: - print("Couldn't open these models:",failed) - table_contents += '' - output=indextemplate.render(modelset=ms, - table_contents=table_contents) - - fh = open(f'{self.base_dir}/{ms.dir}/index.html','w') - fh.write(output) - fh.close() + mp.savefig(f'{self.base_dir}/{fig_out}') + model.write(f'{self.base_dir}/{fits_out}') + # This is supposed to stop complaints about + # too many figures, but actually does not! + mp._plt.close(mp.figure) + output=pagetemplate.render(model=model,name=ms.name, + fitsfilename=f'{modelfile}.fits', + model_explain=EXPLAIN[keyname], + modelfile=modelfile) + fh = open(f'{self.base_dir}/{fig_html}','w') + fh.write(output) + fh.close() + return (ms_dir,True,table_cell,None) + + except FileNotFoundError as fne: + print(fne) + return (ms_dir,False,None,f'{r} {modelfile} : {str(fne)}\n') + except Exception as exc: + print(exc) + return (ms_dir,False,None,f'{r} {modelfile} : {str(exc)}\n') if __name__ == '__main__': # warnings.simplefilter("ignore",DeprecationWarning) -# warnings.simplefilter("ignore",UserWarning) - parser = argparse.ArgumentParser(description='Process CLI.') - parser.add_argument('-q','--quick',help='skip creating plots, just update all_models page',action="store_true") - #TODO figure out how to actuall use this - parser.add_argument('-m','--modelset',help='only do the given modelset',action="store",default=None) + warnings.simplefilter("ignore",SyntaxWarning) + parser = argparse.ArgumentParser(description='Create model webpages for PDR Toolbox website dustem.astro.umd.edu.', prog=sys.argv[0]) parser.add_argument('-k','--kosmatau',help='do the kosma tau models',action="store_true",default=False) + parser.add_argument('-m','--modelset',help='only do the given modelset',action="store",default=None) + parser.add_argument('-q','--quick',help='skip creating plots, just update all_models page',action="store_true") + parser.add_argument('-j','--jobs',help='number of worker processes to use (default: all cores)',action="store",type=int,default=None) args = parser.parse_args() + if args.quick: quick = True else: @@ -217,8 +444,7 @@ def process_modelset(self,n,z,losangle,md,m): manager = Manager() all_models = manager.dict() all_names = manager.dict() - lock = manager.Lock() - p = Page(kosmatau=args.kosmatau) + p = Page(kosmatau=args.kosmatau, modelset=args.modelset) print("using quick = ",quick) - p.make_page(all_models,all_names,lock,quick=quick) + p.make_page(all_models,all_names,quick=quick,jobs=args.jobs) p.write_all_models_page(all_models,all_names) diff --git a/index.html b/index.html index 2e7458e5..901921c0 100755 --- a/index.html +++ b/index.html @@ -71,7 +71,7 @@ incident intensity and cloud density based on our models of PDR emission. One can also fit H2 rovibrational emission excitation diagrams to determine temperature, column density, and ortho-to-para ratio.

-

The current version is 2.6.4 (released April 15, 2026)

+

The current version is 3.0.1 (released August 25, 2026)

Release Highlights

@@ -79,24 +79,25 @@

Release Highlights

    -
  • Alternative Viewing Angle Models
    -

    -Wolfire-Kaufman models are now available for viewing inclination angles from 0 (face-on) to 75 degrees. We also created new notebook showing how to use the new angles.. -

    +
  • Small Magellanic Cloud Models
    +The SMC models have been completely updated using SMC metallicity, abundances, cosmic-ray ionization rate, extinction curve, the improved WK2020 code, and the full range of viewing angles.
    • -
  • Wide variety of dust extinction curves supported
    - Karl Gordon's dust extinction package is now used for fitting visual extinction in excitation diagrams. +
  • More molecules added to excitation fitting
    + Excitation diagrams for C18O, 13C18O, and CH+ can now be fit, with partition functions drawn from HITRAN and EXOMOL, and transition data from Meudon PDR7 code.
    • -
  • Fitting of CO and 13CO excitation diagrams
    • - We have added support for fitting temperatures and column densities of excitation diagrams for CO and 13CO. Users can fit other molecules by providing appropriate transition data. +<<<<<<< HEAD +
  • Users can limit the model ranges with fitting line ratios
    + Limiting the density and radiation field allowable ranges can help prevent unphysical solutions that are not excluded by the data. +
  • Performance improvements
    +Both radiation field/density fitting and excitation diagram fitting now fit multi-pixel maps 2x-11x faster.
    • -
  • Updated notebooks
    -The tutorial notebooks have been revised and a new one added to show use of the alternate viewing angle models. +
  • New and updated notebooks
    + The Example notebooks have been updated and a new notebook added show how to fit H2 excitation on spatial maps.
    • -
  • Bug fixes
    +
  • Other changes and bug fixes

    We have made several bug fixes and addressed requests for enhancment. Thanks to users who reported issues! +href="https://github.com/mpound/pdrtpy/issues?q=is%3Aissue%20closed%3A2026-04-15..2026-09-01%20%20" +>enhancments and bug fixes. Thanks to users who reported issues or asked for new features!

    • @@ -246,7 +247,7 @@

    History

    requested and kept the service running. Single pixel detectors gave way to pixel arrays and the sub-mm science matured. -Since 2020, we have developed and released multiple versions +Since 2020, with new funding, we have developed and released multiple versions of the Python package, retiring the CGI-based scripts.

diff --git a/models.html b/models.html index de991f6c..15b10b1e 100755 --- a/models.html +++ b/models.html @@ -59,15 +59,19 @@

Wolfire/Kaufman Models

The Wolfire/Kaufman models are primarily based on the work of - Tielens & Hollenbach 1985; - + + Tielens & Hollenbach 1985; + + Wolfire et al. 1990; - + Hollenbach et al. 1991; - Kaufman et al. 1999; - and Kaufman et al. 2006. + + Kaufman et al. 1999; + and + Kaufman et al. 2006. For a given set of gas phase elemental abundances and grain properties, each model is described by a constant H nucleus number density, @@ -107,6 +111,11 @@

Wolfire/Kaufman Models

intensity to the infrared dust continuum emission \(I_{FIR}\). More than two observed ratios will of course do a better job of determining unique \(G_0\) and \(n\). +

+Note: +In the Wolfire/Kaufman models, the FIR continuum includes all of the dust emission (including that from PAHs) from 8 μm to 1 mm. This is sometimes called the TIR in the literature rather than FIR. +

+ +
+ +
+
Alternate Viewing Angle Models
The viewing angle models calculate the emitted line intensity along a line-of-sight @@ -194,48 +214,83 @@

2020 Models

Note that the face-on intensity is angle averaged over intensities -emitted from the PDR face as in Tielens & Hollenbach (1985), but the -angle-on intensity is the intensity along the ray at the given angle. +emitted from the PDR face as in + + Tielens & Hollenbach 1985; + +but the angle-on intensity is the intensity along the ray at the given angle.

-

2006 Models

+ +

SMC Models

- In pdrtpy, these are referred to as the wk2006 ModelSet. + In pdrtpy, these are referred to as the smc ModelSet. + The SMC models are primarily based on the work of + + Tielens & Hollenbach 1985; + + Kaufman et al. 2006, + + Hollenbach et al. 2012, + + and + Neufeld & Wolfire 2016. + These use the updates as given for the 2020 Models and modified + for SMC parameters as described in + + Jameson et al. 2018 + + and + + Clark et al. 2025. + + In particular, compared to Galactic, we adopt a + high FUV extinction curve and a low Av/N_H + + (Gordon et al. 2024), + + low gas phase metallicities + + (Toribio San Cipriano et al. 2017), + + a low PAH abundance + + (Sandstrom et al. 2010), + + and a low cosmic-ray ionization rate + + (Abdo et al. 2010). +

+

2006 Models

-These models - are identical to those that were available in the now-deprecated web-based PDR Toolbox. They have metallicity \(Z=1\), + In pdrtpy, these are referred to as the wk2006 ModelSet. +These models have metallicity \(Z=1\), and contain [C I], [C II], [O I], Fe, Si, H2 lines and the 12CO ladder up to \(J=14\rightarrow 13\). For some lines, \(Z=3\) is also available.

-
-
- Spectral lines modeled in PDRT -

Current and future spectral line and metallicity coverage of the PDR Toolbox.

-
-
+

WK Model Parameters

- Our -2006 models -use the standard parameters from Kaufman et al. 1999. Changes for the - 2020 models are listed below. +These models use many of the standard parameters from Kaufman et al. 1999 with later changes related to metallicity, updated abundances, rates, etc. The formation rate of H2 goes as - \(R_{form}~n_{HI}~n\). + \(R_{form} = k_{form}~n_{HI}~n\) cm-3 s-1. The PAH abundance \(X_{PAH}=n_{PAH}/n\).

`` snippet linking to this ratio's page, or + `None` if `success` is `False`. + error : str or None + Description of the failure, or `None` if `success` is + `True`. + """ + key = (n,z,losangle,md,m) + cached = self._ms_cache.get(key) + if cached is None: + ms = ModelSet(name=n,z=z,losangle=losangle,medium=md,mass=m) + if n.startswith("kt2013"): + ms.keyname = "kt2013" + else: + ms.keyname = n + mp = ModelPlot(ms) + # stop complaining about too many figures + mp._plt.rcParams.update({'figure.max_open_warning': 0}) + self._ms_cache[key] = (ms,mp) + else: + ms,mp = cached + + pagetemplatefile = 'model_page_jinja_template.html' + pagetemplate = self.env.get_template(pagetemplatefile) + + try: + #ugly hack + modelfile = ms.table.loc[r]["filename"] + if modelfile == "FEII25p99.fits": + model=ms.get_model(r,unit="erg/(cm3 s ion)") + else: + model=ms.get_model(r) + if "/" in model._title: + #kluge for HII diagnotic files + if "FE" in modelfile or "AR" in modelfile: + model._title += " Emissivity Ratio" #@TODO set modeltype. but need to be able to handle it in Measurement/Modelset + else: + model._title += " Intensity Ratio" + else: + if "FIR" not in model._title and "Surface" not in model._title and "A_V" not in model._title: + #kluge for HII diagnotic files + if "FE" in modelfile or "AR" in modelfile: + model._title += " Emissivity" else: - model._title += " Intensity Ratio" + model._title += " Intensity" + model._title = model._title.replace("$ \mu","$\mu") + model._title = model._title.replace("$\mu$","µ").replace("$_{FIR}$","FIR").replace("$_2$","2").replace("$A_V$","AV").replace("$^{13}$","13").replace("$A_V=0.01$","AV = 0.01") + #.replace("$T_S$","TS") + if "$" in model._title: + print(f"############ OOPS missed some latex {model._title} in {ms.name} {modelfile}") + fig_out = f'{ms_dir}/{modelfile}.png' + fig_html = f'{ms_dir}/{modelfile}.html' + fits_out = f'{ms_dir}/{modelfile}.fits' + f_html = f'{modelfile}.html' + table_cell = f'{model._title}{model._title}
- + - + + + @@ -243,138 +298,155 @@

WK Model Parameters

+ + + + + + + + + - + + + - + + + + + + + + + + + - - - - - - - - - + + + + + - - - - - - - - - + + + + + - + + + - - - + + + + + - - - + + + + + - -
Parameters for 2006 Models
Model Parameters
Parameter SymbolValuewk2020SMCwk2006
Turbulent Doppler velocity \(\delta v_D\) 1.5 km s-11.5 km s-11.5 km s-1
MetallicityZ10.21, 3
Carbon abundance \(X_C\)\(1.4\times10^{-4}\)\(1.6\times10^{-4}\)\(3.2\times10^{-5}\)\(1.4, 4.2\times10^{-4}\)
Oxygen abundance \(X_O\)\(3.0\times10^{-4}\)\(3.2\times10^{-4}\)\(6.4\times10^{-5}\)\(3.0, 9.5\times10^{-4}\)
Silicon abundance \(X_{Si}\) \(1.7\times10^{-6}\)\(3.4\times10^{-7}\)\(1.7, 5.1\times10^{-6}\)
Sulfur abundance \(X_{S}\) \(2.8\times10^{-5}\)\(5.6\times10^{-6}\)\(2.8, 8.4\times10^{-5}\)
Iron abundance \(X_{Fe}\) \(1.7\times10^{-7}\)\(3.4\times10^{-8}\)\(1.7, 5.2\times10^{-7}\)
Magnesium abundance \(X_{Mg}\) \(1.1\times10^{-6}\)\(2.2\times10^{-7}\)\(1.1, 3.3\times10^{-6}\)
Dust abundance relative to diffuse ISM\(\delta_d\)1
FUV dust absorption/visual extinction\(\delta_{UV}\)1.8Fluorine abundance\(X_{F}\)\(1.8\times10^{-8}\)\(3.6\times10^{-9}\)Not included
Dust visual extinction per H\(\sigma_V\)\(5\times10^{-22}\) cm-2
Formation rate of H2 on dust\(R_{form}\)\(3\times10^{-17}\) s-1Helium abundance\(X_{He}\)0.10.10.1
PAH abundance \(X_{PAH}\)\(5\times10^{-7}\)\(2\times10^{-7}\)\(2.6\times10^{-8}\)\(4, 18\times10^{-7}\)
Cloud H density\(n\)\(10^{1} - 10^{7}\) cm-313C abundance\(X_{13C}\)\(3.2\times10^{-6}\)\(6.4\times10^{-7}\)Not included
Incident UV flux\(G_0\)\(10^{-0.5} - 10^{6.5}\) HabingDust abundance relative to diffuse ISM\(\delta_d\)10.11, 3
- - - - - - - - - - - - - - + + + + + - - - + + + + + - - - + + + + + - - - + + + + + - - - + + + + + + + -
Parameters for 2020 Models Changed from 2006
ParameterSymbolValue
Carbon abundance\(X_C\)\(1.6\times10^{-4}\)FUV dust absorption/visual extinction\(\delta_{UV}\)1.83.61.8
Oxygen abundance\(X_O\)\(3.2\times10^{-4}\)Dust visual extinction per H column density\(A_V/N_H\)\(5.26\times10^{-22}\) cm2\(5.35\times10^{-23}\) cm2\(5,15\times10^{-22}\) cm2
Dust visual extinction per H\(\sigma_V\)\(5.26\times10^{-22}\) cm-2Formation rate coefficient of H2 on dust\(k_{form}\)\(6\times10^{-17}\) cm3 s-1\(6\times10^{-18}\) cm3 s-1\(6,18\times10^{-17}\) cm3 s-1
Formation rate of H2 on dust\(R_{form}\)\(6\times10^{-17}\) s-1Cloud H density\(n\)\(10^{1} - 10^{7}\) cm-3\(10^{1} - 10^{7}\) cm-3\(10^{1} - 10^{7}\) cm-3
PAH abundance\(X_{PAH}\)\(2\times10^{-7}\)Incident UV flux\(G_0\)\(10^{-0.5} - 10^{6.5}\) Habing\(10^{-0.5} - 10^{6.5}\) Habing\(10^{-0.5} - 10^{6.5}\) Habing
Viewing Angle \(i_{LOS}\) 0 (face-on) to 75 degrees0 (face-on) to 75 degrees0 (face-on)
- + diff --git a/models/index.html b/models/index.html index a75e7c16..bc43de81 100644 --- a/models/index.html +++ b/models/index.html @@ -36,106 +36,109 @@

Links to All Available ModelSets

To see plots and download individual FITS files for a given ModelSet, click on its ModelSet Description. + - + + + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - + - +
ModelSet name in pdrtpyModelSet Description
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=0
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=75, avlos=27.05, avperp=26.12
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=60, avlos=14.00, avperp=12.12
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=30
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=45, avlos=9.90, avperp=7.00
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=45
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=30, avlos=8.08, avperp=4.04
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=60
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=0, avlos=7.00
wk2020Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=75
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=75
wk2006Wolfire/Kaufman 2006 constant density models, Z=3.0, losangle=0
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=60
wk2006Wolfire/Kaufman 2006 constant density models, Z=1.0, losangle=0
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=45
smcWolfire/Kaufman 2006 limited set of constant density models for Small Magellanic Cloud, Z=0.1, losangle=0
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=30
lmcWolfire/Kaufman 2020 limited set of constant density models for Large Magellanic Cloud, surface chemistry turned off, Z=0.5, losangle=0
smcWolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0, losangle=0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0
kt2020KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0
kt2013wd01-7KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0
kt2013wd01-25KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0
kt2013wd01-21KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0

diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.png index 4938667b..79f0f118 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.png index 5438afdc..a6306d75 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.png index d3d03034..359c29e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.png index 392b0770..b65f8305 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.png index 0dca14e0..453510ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.png index e4551a30..8497a4f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.png index 88e58f26..fdc6208b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.png index 2771899c..1b83452d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.png index 800e6b76..c3758e49 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.png index 5f1d82ae..49536853 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.png index 7b032bb2..e9005f81 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.png index 78506ce0..27fad688 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.png index 55a38066..f8d7702d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.png index 7bab6b0b..700fb934 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.png index dadb9cc7..7d606822 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.png index a063140b..2c9a558a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.png index 5746b069..86028c44 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.png index 938119f7..36f51fe6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.png index 68247e07..dd0b9db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.png index 8c730b4a..a28200b7 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.png index 0d32e9fc..100ad304 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.png index ba65537f..9e58850c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.png index e24e5829..2742a9d1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.png index 99447961..dc7a90c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.png index 0aa2ba83..e31f1d8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.png index ecc6e8f0..3cdcf87d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.png index 87e87f40..81066be1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.png index ec0542ae..532a1a03 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.png index b7426cfb..01e16b7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.png index 2acf1cab..7ebaf442 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.png index f22e201f..3cf6f915 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.png index 0b00df21..1a08ff77 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.png index 65ba0212..a6421686 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.png index 3c160b9e..b0b5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.png index 9fcb52cd..301e161d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.png index a4506dcf..0d8edb28 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.fits b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.fits index cd6f6a70..89bb14f8 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.fits and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.png index 9e6ab321..f08f5176 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png index 6b0fe73a..6a0ab807 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.png index d1c9131c..a0c62691 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.png index 4df1283e..292b285e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png index df3b7377..c58ccd3c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.png index f3932885..275be16a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/index.html b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/index.html index a68a4eef..a79ddee0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M0.1/index.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.png index 4938667b..79f0f118 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.png index 5438afdc..a6306d75 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.png index d3d03034..359c29e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.png index 392b0770..b65f8305 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.png index 0dca14e0..453510ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.png index e4551a30..8497a4f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.png index 88e58f26..fdc6208b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.png index 2771899c..1b83452d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.png index 800e6b76..c3758e49 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.png index 5f1d82ae..49536853 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.png index 7b032bb2..e9005f81 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.png index 78506ce0..27fad688 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.png index 55a38066..f8d7702d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.png index 7bab6b0b..700fb934 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.png index dadb9cc7..7d606822 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.png index a063140b..2c9a558a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.png index 5746b069..86028c44 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.png index 938119f7..36f51fe6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.png index 68247e07..dd0b9db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.png index 8c730b4a..a28200b7 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.png index 0d32e9fc..100ad304 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.png index ba65537f..9e58850c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.png index e24e5829..2742a9d1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.png index 99447961..dc7a90c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.png index 0aa2ba83..e31f1d8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.png index ecc6e8f0..3cdcf87d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.png index 87e87f40..81066be1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.png index ec0542ae..532a1a03 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.png index b7426cfb..01e16b7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.png index 2acf1cab..7ebaf442 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.png index f22e201f..3cf6f915 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.png index 0b00df21..1a08ff77 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.png index 65ba0212..a6421686 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.png index 3c160b9e..b0b5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.png index 9fcb52cd..301e161d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.png index a4506dcf..0d8edb28 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.fits b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.fits index d158dadd..64c69c9a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.png index 20f41b5a..2e90f9b8 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png index 6b5d762c..4a52c2f6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.png index d1c9131c..a0c62691 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.png index 4df1283e..292b285e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png index 8e826bb8..41d7fafa 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.png index f3932885..275be16a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/index.html b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/index.html index a0e26a95..420b0e3d 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1.0/index.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.png index 4938667b..79f0f118 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.png index 5438afdc..a6306d75 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.png index d3d03034..359c29e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.png index 392b0770..b65f8305 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.png index 0dca14e0..453510ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.png index e4551a30..8497a4f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.png index 88e58f26..fdc6208b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.png index 2771899c..1b83452d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.png index 800e6b76..c3758e49 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.png index 5f1d82ae..49536853 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.png index 7b032bb2..e9005f81 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.png index 78506ce0..27fad688 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.png index 55a38066..f8d7702d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.png index 7bab6b0b..700fb934 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.png index dadb9cc7..7d606822 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.png index a063140b..2c9a558a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.png index 5746b069..86028c44 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.png index 938119f7..36f51fe6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.png index 68247e07..dd0b9db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.png index 8c730b4a..a28200b7 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.png index 0d32e9fc..100ad304 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.png index ba65537f..9e58850c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.png index e24e5829..2742a9d1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.png index 99447961..dc7a90c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.png index 0aa2ba83..e31f1d8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.png index ecc6e8f0..3cdcf87d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.png index 87e87f40..81066be1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.png index ec0542ae..532a1a03 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.png index b7426cfb..01e16b7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.png index 2acf1cab..7ebaf442 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.png index f22e201f..3cf6f915 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.png index 0b00df21..1a08ff77 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.png index 65ba0212..a6421686 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.png index 3c160b9e..b0b5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.png index 9fcb52cd..301e161d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.png index a4506dcf..0d8edb28 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.fits b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.fits index 17cfcb58..b586b0c1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.png index 4e097737..7e9513d3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png index af413826..80dba820 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.png index d1c9131c..a0c62691 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.png index 4df1283e..292b285e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png index 45b0482b..38359901 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.png index f3932885..275be16a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/index.html b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/index.html index 2fc454e3..232b9918 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M10.0/index.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.png index 4938667b..79f0f118 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.png index 5438afdc..a6306d75 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.png index d3d03034..359c29e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.png index 392b0770..b65f8305 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.png index 0dca14e0..453510ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.png index e4551a30..8497a4f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.png index 88e58f26..fdc6208b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.png index 2771899c..1b83452d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.png index 800e6b76..c3758e49 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.png index 5f1d82ae..49536853 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.png index 7b032bb2..e9005f81 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.png index 78506ce0..27fad688 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.png index 55a38066..f8d7702d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.png index 7bab6b0b..700fb934 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.png index dadb9cc7..7d606822 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.png index a063140b..2c9a558a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.png index 5746b069..86028c44 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.png index 938119f7..36f51fe6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.png index 68247e07..dd0b9db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.png index 8c730b4a..a28200b7 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.png index 0d32e9fc..100ad304 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.png index ba65537f..9e58850c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.png index e24e5829..2742a9d1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.png index 99447961..dc7a90c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.png index 0aa2ba83..e31f1d8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.png index ecc6e8f0..3cdcf87d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.png index 87e87f40..81066be1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.png index ec0542ae..532a1a03 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.png index b7426cfb..01e16b7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.png index 2acf1cab..7ebaf442 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.png index f22e201f..3cf6f915 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.png index 0b00df21..1a08ff77 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.png index 65ba0212..a6421686 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.png index 3c160b9e..b0b5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.png index 9fcb52cd..301e161d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.png index a4506dcf..0d8edb28 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.fits b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.fits index a73e5b8f..70342b4d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.png index 604469c3..464b41cf 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png index 38992aa3..1a4f5c94 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.png index d1c9131c..a0c62691 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.png index 4df1283e..292b285e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png index 35a28357..1a305fd6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.png index f3932885..275be16a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/index.html b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/index.html index 2148439e..9e0d5443 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M100.0/index.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.png index 4938667b..79f0f118 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.png index 5438afdc..a6306d75 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.png index d3d03034..359c29e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.png index 392b0770..b65f8305 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.png index 0dca14e0..453510ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.png index e4551a30..8497a4f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.png index 88e58f26..fdc6208b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.png index 2771899c..1b83452d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.png index 800e6b76..c3758e49 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.png index 5f1d82ae..49536853 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.png index 7b032bb2..e9005f81 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.png index 78506ce0..27fad688 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.png index 55a38066..f8d7702d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.png index 7bab6b0b..700fb934 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.png index dadb9cc7..7d606822 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.png index a063140b..2c9a558a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.png index 5746b069..86028c44 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.png index 938119f7..36f51fe6 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.png index 68247e07..dd0b9db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.png index 8c730b4a..a28200b7 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.png index 0d32e9fc..100ad304 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.png index ba65537f..9e58850c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.png index e24e5829..2742a9d1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.png index 99447961..dc7a90c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.png index 0aa2ba83..e31f1d8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.png index ecc6e8f0..3cdcf87d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.png index 87e87f40..81066be1 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.png index ec0542ae..532a1a03 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.png index b7426cfb..01e16b7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.png index 2acf1cab..7ebaf442 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.png index f22e201f..3cf6f915 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.png index 0b00df21..1a08ff77 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.png index 65ba0212..a6421686 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.png index 3c160b9e..b0b5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.png index 9fcb52cd..301e161d 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.png index a4506dcf..0d8edb28 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.fits b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.fits index 9a69586a..e873680c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.png index adb3a67f..171e9c2c 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html index 43517e0a..f338912d 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png index 0fd8949a..23f034db 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.png index d1c9131c..a0c62691 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.png index 4df1283e..292b285e 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html index f811d97e..ac8525d3 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png index 0c8d173c..57e71a9b 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.png index f3932885..275be16a 100644 Binary files a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/index.html b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/index.html index 5ba5ce92..da1da77c 100644 --- a/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/index.html +++ b/models/kt2013wd01-21_Z1.0_clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.fits index 34802ccc..794c6fee 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.html index 500a2af6..e72a482e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.png index db1d329e..7e721bae 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.png index 2c005531..d60b4d3b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.fits index 0cc48d3f..d85f75e4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.html index 0f700c85..3c749595 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.png index 070b2faa..bf8bd8cb 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.fits index d8e62976..8fd9c89c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.html index fc3cd676..28f04ce1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.png index cd868fb7..ea3f016b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.png index abae6651..43eaf33f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.png index 1887708c..e7f1c01b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.png index 21567bcb..5870884b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.png index 05400979..6ce50f5c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.png index 35b70d55..7ea94cb3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.png index 0f814536..ce68e61f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.png index 58aa1367..23c0b25a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.fits index 1c1401d7..0d30165a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.html index 8a5a473d..c235e0f9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.png index f94d4deb..6b361fb3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.fits index dc0711c8..6e69a984 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.html index d3fae0d1..e88e5ab8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.png index 96cde700..7a3db18d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.png index 9e4ea6dd..2b00580f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.png index 7bcdf5e6..c932cfee 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.png index e8292c2a..69df3fef 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.fits index 16f6c813..d38d1d02 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.html index cbddb2d7..8868e284 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.png index f3ef5528..37078dfd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.png index d5440ce5..bc26a418 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.png index fc3bb980..ca2ab410 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.fits index 18e0f98c..15a8e3fb 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.html index ed8165cb..6ce2eb7a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.png index e46732ff..a9245d16 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.png index c5107841..37a3cddc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.png index dde03fff..27ea71cc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.fits index 840acd0e..0060b277 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.html index 51d65276..c2cd6859 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.png index b1d81722..207f50a0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.png index dc47ac3c..5365be04 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.png index 0d1965cf..03feca5d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.fits index 11f4f830..e0cf453b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.html index 16d60b99..2b848d1e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.png index 15267978..dfbeecc6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.png index b2d37b02..6b1551ea 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.png index 33c58df9..bcee5f51 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.fits index b8f9736b..7ae65903 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.html index e211e374..5bcaec29 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.png index d1388185..155fbffa 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.png index 85f53917..f42eff87 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.png index 97728b29..ac37756c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.png index 2ea9e5a0..d36f7bde 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.fits index e9d1c6c4..1f0e4090 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.html index 91bc8f49..1623bb63 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.png index 9d1490b3..b86add35 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.png index fc3faf6f..d2c06374 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.png index 53b3b520..3a62e885 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.fits index 5fd2c43d..65ab2ff5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.html index c3bcae54..796a1d9c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.png index f0b8f591..325dcdf2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.fits index fd48c198..12f3bec8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.html index 81602c75..85553cca 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.png index 60d54386..87e63048 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.png index 577fa163..f09b0970 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.png index 5abc0813..a23949d9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.png index 250a8247..c8beab38 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.fits index c6ca9a65..5766b495 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.html index 21133957..d66e99f8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.png index 9787785e..3db7a6e3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.png index e65cfe29..59a3e212 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.png index 1f970f49..422378f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.png index b1e4ec49..5a4459dd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.png index 6a4c3ea8..461fc0f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.png index 8f685e77..760e72db 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.fits index 712e0a65..a181d1e9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.html index 46dc6e82..05d45d59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.png index 96748ec2..427b9462 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.png index 4a0ac49a..94bf6d40 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.png index fe704aa1..034c929b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.fits index 5641ed90..ff5ee147 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.html index ac0b3938..15817f49 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.png index 8abbeba6..294424a4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.png index 0869769c..49ed8f6e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.png index 60ebec4b..64a374b0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.fits index a042d3a9..b7581475 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.html index b587e6e3..63323e57 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.png index 3dd9735c..3a51d1fa 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/CP32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.fits index 9f529f0c..465b9e6b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.png index 9e6ab321..f08f5176 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.fits index 7fa8af36..e5c14b25 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.html index 70b496e0..a4e3e888 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.png index b9d2429b..bcfcdfd8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png index dedb01ee..ec046051 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.fits index 8fabdf49..f3119710 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.html index bd5d9298..f0cde142 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.png index c0d518a3..d1b6c157 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.png index bf6676b6..082c279f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.png index b27b2980..00b1d946 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.fits index 7881c97d..45c7bc01 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.html index 7dd985d4..0107d524 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.png index 950e73b4..a0f167ac 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png index 50afbaf6..b70b7dba 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.fits index 009575b5..fa1a7c2f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.html index cf609828..7fc3e77b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.png index f84e94ee..eb08ab65 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.png index 98a2f085..ccd30e87 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.html index cd6a8fe9..8b80c393 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.png index b350d016..a2b12c43 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/Ts.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/index.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/index.html index 1dd3d75b..cfdc4bd4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/index.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.fits index b7e2aa29..3fb35c17 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.html index 500a2af6..e72a482e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.png index f97c42ab..ccb7fa18 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.png index 47132001..374a48d3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.fits index f8f940a2..6b2b078a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.html index 0f700c85..3c749595 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.png index 1a425fc9..08d78622 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.fits index 550f5262..a726b9e2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.html index fc3cd676..28f04ce1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.png index 84d881aa..5b65a296 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.png index 0b127bf9..e837c97c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.png index ee4af63c..d81937f8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.png index db402cb8..7d1a91d3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.png index 6c3e681b..682ae3b3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.png index a6f4dca5..9707f24a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.png index 7b1120b2..5c7ae9b6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.png index 58de1af4..0740e573 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.fits index af0eeb6e..7ce5e295 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.html index 8a5a473d..c235e0f9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.png index ec12808a..9fd1d70d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.fits index 0f2abfca..a6cf0e04 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.html index d3fae0d1..e88e5ab8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.png index 947bb6e4..d1bb8e73 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.png index c7bd10f5..c77002a9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.png index 8e252a53..655657ce 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.png index 16a634a2..dca363cf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.fits index 755c72f0..7ef5a0a2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.html index cbddb2d7..8868e284 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.png index 7a81ee9e..70de18fc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.png index f0c6161e..1afca880 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.png index a0bec8cf..857de50a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.fits index 0d59c01f..66158252 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.html index ed8165cb..6ce2eb7a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.png index d11c3304..660e0096 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.png index 4fcd6f01..55948666 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.png index 14d12962..ec72f2a1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.fits index 4c04bfa0..5630332d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.html index 51d65276..c2cd6859 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.png index a8053e6b..63073358 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.png index d29861d1..07d62c68 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.png index 375a9095..e64b732b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.fits index fabbaf44..c78519de 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.html index 16d60b99..2b848d1e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.png index 18ca6980..0825bcc9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.png index 908fdf91..151a5583 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.png index 247df875..c081c5d2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.fits index dce7ff8a..e16c807e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.html index e211e374..5bcaec29 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.png index 9e1cdb4b..a5dc2693 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.png index fdeb9edf..09a360f0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.png index 7175dfd2..4475d66c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.png index 3704c329..42aef720 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.fits index 6f750811..9a42f79c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.html index 91bc8f49..1623bb63 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.png index 9138e5cc..2735607e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.png index 0cb9d5ef..82535056 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.png index 63618204..c113b94a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.fits index eb80a485..2c9244bc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.html index c3bcae54..796a1d9c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.png index b7c3af45..8c3f224a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.fits index 5d8a3b2c..9c2383ef 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.html index 81602c75..85553cca 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.png index 938c8ffe..99769afe 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.png index 3880ab73..da494677 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.png index fae719e6..4abf208a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.png index 398690d7..8b66ac25 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.fits index 64313e05..bd19beab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.html index 21133957..d66e99f8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.png index bace65a6..5706008a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.png index 86c6e2cc..9e319b62 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.png index 28e49929..2ab83db3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.png index d0780cab..46be3fdc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.png index 42d1eaac..d16694a5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.png index 387f61cf..7b01c753 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.fits index 43877a62..d6c30f36 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.html index 46dc6e82..05d45d59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.png index dbc062e3..c17eedab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.png index 851c48fa..28ee09fd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.png index 05fb03bf..54281a02 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.fits index 0b1ad8b0..b920deb9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.html index ac0b3938..15817f49 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.png index febe3035..7ed410ee 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.png index ccc8da11..89284dfa 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.png index 7e451f54..7236a55b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.fits index cc007657..5043091b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.html index b587e6e3..63323e57 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.png index 91c30ec7..8c3db2f1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/CP32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.fits index 9f71eca1..c7871991 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.png index 20f41b5a..2e90f9b8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.fits index 9855c694..877bcf5e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.html index 70b496e0..a4e3e888 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.png index 96b1d5f5..362ba6ca 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png index a516dcaf..78ae65eb 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.fits index 5b7a7973..8d50633f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.html index bd5d9298..f0cde142 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.png index ace94ce7..c035902c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.png index 35251761..9baa23e8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.png index a1ff44fe..4896a1c4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.fits index 87975695..dd6393fa 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.html index 7dd985d4..0107d524 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.png index d40cfd85..4169b2f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png index 7802dbc6..fa7c856a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.fits index f6e372ce..5fb7f8bf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.html index cf609828..7fc3e77b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.png index 1bbc98df..314dd2c2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.png index 648244ce..2cfaf60e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.html index cd6a8fe9..8b80c393 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.png index f06677ee..8475174a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/Ts.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/index.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/index.html index bf51cb41..4042c2ba 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/index.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.fits index c451ecd0..9a22b479 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.html index 500a2af6..e72a482e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.png index b1543c4b..4a2cbaab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.png index cfd53f90..a576f3b2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.fits index 9f329af6..24fe9a44 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.html index 0f700c85..3c749595 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.png index bffbb1ad..c1886194 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.fits index fe4aa6bc..44363a39 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.html index fc3cd676..28f04ce1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.png index a8be633a..f92e498e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.png index 7e31efa1..de1b85cc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.png index 856d7df0..b487865d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.png index 041406d7..381636e7 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.png index 991f6a4f..33c9e46a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.png index 24485952..f7f69a54 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.png index 60de0dd1..30cf13dc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.png index a5fd4221..36d410a2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.fits index 4bb73027..57d7ae83 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.html index 8a5a473d..c235e0f9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.png index 3cd0855e..1ecdeb83 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.fits index 5210883d..1b9fa97f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.html index d3fae0d1..e88e5ab8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.png index 88daf3c4..57d825c4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.png index 66e486d4..f82366c7 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.png index 53d6cb18..931c295a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.png index af268fc6..899cf4ec 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.fits index c8bfc266..70840cc6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.html index cbddb2d7..8868e284 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.png index 32dabd92..245fec0a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.png index 9ac6d9ac..2ff8cfd2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.png index 5c85b5c7..89af6e78 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.fits index e21d24ce..5971b109 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.html index ed8165cb..6ce2eb7a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.png index c1f957c8..b10844b4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.png index 2a5cb65f..2df97fa5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.png index 12eb656c..4da2c5fc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.fits index 368d5873..179bec3d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.html index 51d65276..c2cd6859 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.png index dc6e8525..e41762c9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.png index eba1e003..0fd0952a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.png index 95123f25..689cca55 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.fits index 8f8b586b..393586c9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.html index 16d60b99..2b848d1e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.png index 8bfd4c79..4d94e2d2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.png index 13991422..ff8cd0b9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.png index 9be4e859..cdd4a83b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.fits index 87ae3515..04130af5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.html index e211e374..5bcaec29 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.png index 7476e6e3..7c99c377 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.png index 27dc7b9b..8716c996 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.png index df29ddbb..57923445 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.png index 99c34ae7..69533104 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.fits index f7618037..c817c878 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.html index 91bc8f49..1623bb63 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.png index 3dc09dfb..d976d42d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.png index 28628cf4..14f4e085 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.png index 86eb1080..e3f56f7a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.fits index c389fec6..227b2cbc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.html index c3bcae54..796a1d9c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.png index 46e31eee..e0a6cc75 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.fits index 51b2e1fb..226517bb 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.html index 81602c75..85553cca 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.png index 08265238..14c8ac96 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.png index 66925c41..6d048070 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.png index f4e96dd4..860cc324 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.png index 73b31387..24e25d31 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.fits index 7f0dfe98..38880480 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.html index 21133957..d66e99f8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.png index 5ac38774..bf9b1dfd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.png index 309f8287..bfac0b40 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.png index cbd1ea19..1cde710b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.png index e2498024..94cb082a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.png index afafb9b3..b7f0c466 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.png index a0c94229..1d61d074 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.fits index 9bbca263..1f1c75fe 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.html index 46dc6e82..05d45d59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.png index f145e710..cd3e03fc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.png index 22e9ab32..dba41453 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.png index 30612d05..17061ae4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.fits index 9663c77b..1879bb4a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.html index ac0b3938..15817f49 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.png index ece95eec..fa2436ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.png index 4cb3d79f..adc84891 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.png index 7d9b6acc..ebce92e6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.fits index 8cc38ef7..64bb1082 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.html index b587e6e3..63323e57 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.png index b59b9077..3cb8d72b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/CP32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.fits index 637e26bc..4b737709 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.png index 4e097737..7e9513d3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.fits index 271e23ba..652b0670 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.html index 70b496e0..a4e3e888 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.png index 147b6c96..b202e54a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png index 4fff3372..6d194017 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.fits index 6d36fbf8..9137219b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.html index bd5d9298..f0cde142 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.png index 545da4f9..7c894bbf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.png index e67b2c2b..99ffb211 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.png index 3e6f1a57..721150ea 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.fits index ef27f711..d5e6d92e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.html index 7dd985d4..0107d524 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.png index 4d9fd246..fdc5031b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png index 5d2f9aaf..c503349b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.fits index 057bbe4f..7de03a79 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.html index cf609828..7fc3e77b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.png index 0d22c2f3..8df5c809 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.png index 00f5e0ab..ba3d3875 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.html index cd6a8fe9..8b80c393 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.png index f0b7d240..6d08de45 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/Ts.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/index.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/index.html index 47b55d40..3d03a01c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/index.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.fits index 09edd3ec..29b59d71 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.html index 500a2af6..e72a482e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.png index 989a3996..1ad297a5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.png index 003fe6d9..a3aa3980 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.fits index 7551274b..5179f11b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.html index 0f700c85..3c749595 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.png index bae2967e..25e7e235 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.fits index efbebf16..ab780c91 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.html index fc3cd676..28f04ce1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.png index c1ce0152..c0bbf36c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.png index 87c1ef98..44f88f2f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.png index ad2729c9..d4221845 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.png index 02a16b80..ef031a99 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.png index c476ae64..3584d208 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.png index 52d00fdf..e219f909 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.png index dfd4b33e..47c5aae8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.png index eba120a1..fb8758ce 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.fits index 2d85d14a..12d083fc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.html index 8a5a473d..c235e0f9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.png index 794ac969..321299dd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.fits index 743c16de..9c773cdd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.html index d3fae0d1..e88e5ab8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.png index a64e0687..a4ff3285 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.png index 0fb05afb..3f0ee9d9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.png index e0029a39..c5d27d19 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.png index aaf4d60f..d88e0b6b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.fits index 651689c4..77b6596c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.html index cbddb2d7..8868e284 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.png index a09b85a2..d63b8d23 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.png index afc54ec4..22839242 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.png index b5da42be..67248cb5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.fits index 70208b0a..1af02f8b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.html index ed8165cb..6ce2eb7a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.png index daf3a4d5..7ad34063 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.png index 0881e03e..c1ce8256 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.png index 0d8555c9..2dd5dff2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.fits index 48ea8265..55b9b32c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.html index 51d65276..c2cd6859 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.png index 2a7c20d0..9c5354d2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.png index be054369..d3007a00 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.png index 5d507333..2c793585 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.fits index dd84dc42..bcd3d5a7 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.html index 16d60b99..2b848d1e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.png index 26a81812..082e91a9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.png index 71a6391d..126415ac 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.png index 4619b68b..4e075c52 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.fits index 797b5777..0e3b9ef4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.html index e211e374..5bcaec29 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.png index c534b089..2f6d4efc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.png index 5447f8f1..73de96a3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.png index 2d40de7d..c3f25cc9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.png index ba1bae5b..c043980a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.fits index f37d4641..0ec3036e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.html index 91bc8f49..1623bb63 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.png index 25ea7d1c..585d7ebf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.png index e3d27527..ebf7a8c6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.png index 5dc9c455..be8f77dc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.fits index 276056f9..0da66597 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.html index c3bcae54..796a1d9c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.png index e4892365..702c5ee4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.fits index feca3bcd..ad2f4168 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.html index 81602c75..85553cca 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.png index cd2f3ae5..49f93554 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.png index 0f1df3fd..49dd5da4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.png index eeba9846..1a0c187e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.png index 4dc3d9b3..e14eb4d9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.fits index 820cbbc5..6b375d9e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.html index 21133957..d66e99f8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.png index 4454dec9..e8f7c55f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.png index fe684f06..456cb8b4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.png index 21a32ed1..9c6a9314 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.png index bb9d2e58..3432140d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.png index 00dea32a..32271a60 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.png index a16b4b41..9d8546ca 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.fits index 95cb4211..9f06f225 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.html index 46dc6e82..05d45d59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.png index 0fac9bd2..213e4740 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.png index 7ba4ad57..7d92f58b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.png index d0389d65..af06da9e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.fits index af5b4dc2..7f37c876 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.html index ac0b3938..15817f49 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.png index 390b91fb..b79a778b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.png index f5540f20..f8cadfe0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.png index e1f6b06c..f32ab41c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.fits index 783829e8..cdd04ce6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.html index b587e6e3..63323e57 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.png index 000c147d..9c05545d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/CP32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.fits index 8b593f45..6b9b758e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.png index 604469c3..464b41cf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.fits index 8afa155c..6c5bab7f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.html index 70b496e0..a4e3e888 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.png index e38d19a7..95bd768e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html index a3b2eae3..e01c15ba 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png index 74eea63b..26f3a564 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.fits index 3628b71d..573138bd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.html index bd5d9298..f0cde142 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.png index 9ba95b6a..c0ef3dd2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.png index 65f528fc..2e923705 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.png index cc04bfea..49abfc13 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.fits index 42990bbe..cd26516e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.html index 7dd985d4..0107d524 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.png index ee13b8ee..86d01f34 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html index 6b186a28..0ff85c7b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png index 3b713aae..782e522a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.fits index 6e9e2d33..b94e3a8d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.html index cf609828..7fc3e77b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.png index e2df0bea..ec91ac2f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.png index ba9c4c64..ad6ab7b1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.html index cd6a8fe9..8b80c393 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.png index 8725517f..66217d2c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/Ts.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/index.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/index.html index 50b4e638..a29d19bc 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/index.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.fits index cd74ead2..84fb4f35 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.html index 500a2af6..e72a482e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.png index 64c8cf8a..3f3206f2 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.html index 1c908266..6af17b59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.png index a745616d..4090275f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.fits index f18b92d2..8062d344 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.html index 0f700c85..3c749595 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.png index 20760fe3..080630ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.fits index 78e8ece8..14b1352b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.html index fc3cd676..28f04ce1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.png index 11583b9c..ae3b8397 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.html index 9aed5c64..c5beae3e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.png index c1297809..9b366892 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.html index c7231f58f..192c6097 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.png index ea777eef..5ad5214e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.html index cc5e7c65..a7c61d83 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.png index 56861ab4..89e22823 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.html index 038f077a..2dc0c83a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.png index b7656287..ae900dc4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.html index 90c9ca5b..fa30cd2a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.png index 6e9d2fd9..a9e2bfdf 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.html index 159c8b6a..3eaebe52 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.png index ef560811..b8d40c32 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.html index 20c4eb11..e3a3e816 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.png index de3b5bcb..23cd71e1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.fits index a6b4235e..a29fe91f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.html index 8a5a473d..c235e0f9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.png index 947d2308..e3ba4fa8 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.fits index 105485ed..c09ec9ba 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.html index d3fae0d1..e88e5ab8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.png index 9e2d5820..131956b1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.html index be96a1fb..a1f94362 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.png index ac682e87..89cb9a34 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.html index a77333e3..8f388bb6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.png index 3520d21d..253322bd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.html index 356d51d8..5e70e5b1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.png index cb58dd8d..8ea79621 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.fits index c8c4f897..67f135c9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.html index cbddb2d7..8868e284 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.png index 7da03c62..86b1aaa6 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html index ab99b620..edf4dd89 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png index 679ae2ad..bd36a126 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html index e094141f..974df9cd 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png index c9eadde6..2627b519 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.fits index 4b8faf6d..6c83b04e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.html index ed8165cb..6ce2eb7a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.png index d67b23ae..d1750c7e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html index 5b049a05..fa87acf1 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png index ef34e39e..f8f1ccf9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html index e30a213e..b4cdcd27 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png index 06abda59..9b129834 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.fits index 1340f272..75f6c056 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.html index 51d65276..c2cd6859 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.png index 34c5dfd6..2c3ca38a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html index 84f30133..8e14b17c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png index decaa202..a142d4c0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html index 19860867..bb164e39 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png index 4e415573..6965fb03 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.fits index 06890ca7..85c47c47 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.html index 16d60b99..2b848d1e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.png index 45c8dbfb..f9377343 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html index 9072d2c6..de3fdd26 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png index f6911af6..b0b263dc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html index 349e8f2f..17f596eb 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png index ad7ae154..2e54bfb1 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.fits index b7fc72af..c9cc3993 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.html index e211e374..5bcaec29 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.png index 5273451a..67b65290 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.html index caf96459..46f9f5ac 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.png index 6a3db1f5..34b0f507 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.html index 4976aff0..0a89c381 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.png index 3bdd908e..73b11420 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.html index ba05e780..1664584e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.png index fceed817..f1c15125 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.fits index a00d2cd7..0d07d6ee 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.html index 91bc8f49..1623bb63 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.png index 2c838d7d..830159de 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.html index 4c4a15eb..024e88b8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.png index 46cc2f06..e5957912 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.html index 504f89f6..0315200a 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.png index e43f5368..c6f53d5e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.fits index c843b1b0..d01b4a79 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.html index c3bcae54..796a1d9c 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.png index d4bb65e0..f6319f1d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.fits index bbd1b551..9f9065dd 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.html index 81602c75..85553cca 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.png index 493af177..99667a53 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.html index d9c5b1d2..4bb5a861 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.png index df661629..07daa4ac 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.html index 0ab4fe24..beb111ae 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.png index 6730ef31..73bfc377 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.html index 6be2df2d..d0a57ea0 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.png index 232f26fd..bf08d1f9 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.fits index 3490cbaf..d35b1950 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.html index 21133957..d66e99f8 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.png index 678ab71e..9a20b522 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.html index 62f0908d..5a4ebe6f 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.png index 85ae1437..08b01702 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.html index f08184ae..8fc245f7 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.png index 64cffdd5..ac40fe32 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.html index 7e576ed7..64aa7ae2 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.png index df36e6a8..cd921fdc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.html index 0d1d1953..b07fa8b4 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.png index b2e4dd17..0a0ecb77 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.html index ffa75761..23a74352 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.png index d79a20ca..02fdf095 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.fits index e09ca6a0..5fb298c3 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.html index 46dc6e82..05d45d59 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.png index 9b7bc01a..9a4166ca 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.html index fb8b0a5e..727c2af6 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.png index 3f208159..d5106a2d 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.html index 7d0c3627..e930ca5e 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.png index 610eb645..0e38aeb4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.fits index c126bc17..72d7fe9a 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.html index ac0b3938..15817f49 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.png index 5c8694c6..b35c95f5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.html index 075f7f56..f3261a85 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.png index 07306fae..d9a4f09f 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.html index 880632ff..9a79e3d9 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.png index eeac70c1..c791c8bc 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.fits index e27e0860..c30260be 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.html index b587e6e3..63323e57 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.png index d088374b..ad4448d0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/CP32.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.fits index b68b306f..efe1a716 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.html index e446c08f..bf25cf31 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.png index adb3a67f..171e9c2c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits index 1373e41b..f83548b4 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.html index 70b496e0..a4e3e888 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.png index 3d9ae718..8f3cd601 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html index 43517e0a..f338912d 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png index c53dcbef..911f0417 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.fits index c0749a76..617a8fd5 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.html index bd5d9298..f0cde142 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.png index a9debab4..b1ed30c0 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.html index 1cbed7a3..8c4bb041 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.png index 89a24289..d6d8063b 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.html index 7d35b716..d1e48f35 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.png index c38de2b2..6fe924ab 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits index 185a2065..46f2bb15 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.html index 7dd985d4..0107d524 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.png index 08150700..e3255217 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html index f811d97e..ac8525d3 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png index 70e3d431..0c6f503c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.fits b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.fits index fb592dcc..6689e51e 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.fits and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.fits differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.html index cf609828..7fc3e77b 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.png index 5478967a..4fb78cdb 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.html index fc0bc008..f21a7154 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.png index 40efe2f9..6fab5dba 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.html index cd6a8fe9..8b80c393 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.png b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.png index 73d9aaa1..2650501c 100644 Binary files a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.png and b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/Ts.png differ diff --git a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/index.html b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/index.html index 4b9e2c17..f7386c17 100644 --- a/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/index.html +++ b/models/kt2013wd01-21_Z1.0_non-clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=4.0, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-21 kt2013wd01-21 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.png index 9668f43c..a1070b95 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.png index 75bb6115..f96d245a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.png index 53c634a1..31faee8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.png index 3cbc72c3..958ff385 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.png index 5a974631..c99c2da3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.png index 4bdb3736..9bf18142 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.png index f5e60728..528eb0b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.png index 0dfb26c8..0282952d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.png index 17c57296..1fd48485 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.png index 553e2fec..f9b8c5d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.png index d76fdda9..32c39fee 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.png index 8686b255..5439c6b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.png index 3c5739b8..bf6df997 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.png index 51a73200..40e2c9ff 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.png index f0dbeac8..45257270 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.png index c54a0940..ec2b8fd3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.png index cfadb631..e1fa758d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.png index 846af902..5fbbfb79 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.png index 2cac36fa..3056b82c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.png index 17cf32da..04efdd54 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.png index 3c1e1b7f..b63ed40c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.png index 6bfc2a56..f6e6f78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.png index ecf91e12..4072fcb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.png index 050a75a1..94085900 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.png index e3f8a9d9..a6b86b80 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.png index 95ebc0fb..1703efac 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.png index 6e29e9c0..6722a8bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.png index f3aa4f80..28899910 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.png index 1a671a6a..e732acc5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.png index 327e73bb..5476274f 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.png index ad74dda8..95342093 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.png index 6d907e12..000e2b9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.png index 9699ad29..994f2ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.png index 2af6ae5c..25c75afa 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.png index 4dde157f..5382a460 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.png index 4a38d57f..7894a136 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.fits b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.fits index 5d83172a..129bfb71 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.fits and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.png index ff28069f..a9e031e3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png index df0ce296..11a7853b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.png index 43be7749..e98b0a62 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.png index a0f7f574..58dba519 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png index a3da0c59..ab0a7e4b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.png index 0af1b7da..1960c6c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/index.html b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/index.html index 2539e4f3..59c4a722 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M0.1/index.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.png index 9668f43c..a1070b95 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.png index 75bb6115..f96d245a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.png index 53c634a1..31faee8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.png index 3cbc72c3..958ff385 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.png index 5a974631..c99c2da3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.png index 4bdb3736..9bf18142 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.png index f5e60728..528eb0b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.png index 0dfb26c8..0282952d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.png index 17c57296..1fd48485 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.png index 553e2fec..f9b8c5d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.png index d76fdda9..32c39fee 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.png index 8686b255..5439c6b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.png index 3c5739b8..bf6df997 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.png index 51a73200..40e2c9ff 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.png index f0dbeac8..45257270 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.png index c54a0940..ec2b8fd3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.png index cfadb631..e1fa758d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.png index 846af902..5fbbfb79 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.png index 2cac36fa..3056b82c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.png index 17cf32da..04efdd54 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.png index 3c1e1b7f..b63ed40c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.png index 6bfc2a56..f6e6f78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.png index ecf91e12..4072fcb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.png index 050a75a1..94085900 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.png index e3f8a9d9..a6b86b80 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.png index 95ebc0fb..1703efac 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.png index 6e29e9c0..6722a8bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.png index f3aa4f80..28899910 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.png index 1a671a6a..e732acc5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.png index 327e73bb..5476274f 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.png index ad74dda8..95342093 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.png index 6d907e12..000e2b9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.png index 9699ad29..994f2ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.png index 2af6ae5c..25c75afa 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.png index 4dde157f..5382a460 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.png index 4a38d57f..7894a136 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.fits b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.fits index f274aa36..aa117c39 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.png index fcfca894..ce835e1e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png index fe8e095a..27906a2b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.png index 43be7749..e98b0a62 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.png index a0f7f574..58dba519 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png index 38635865..abe1097e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.png index 0af1b7da..1960c6c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/index.html b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/index.html index c966c890..c2829c80 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1.0/index.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.png index 9668f43c..a1070b95 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.png index 75bb6115..f96d245a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.png index 53c634a1..31faee8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.png index 3cbc72c3..958ff385 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.png index 5a974631..c99c2da3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.png index 4bdb3736..9bf18142 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.png index f5e60728..528eb0b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.png index 0dfb26c8..0282952d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.png index 17c57296..1fd48485 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.png index 553e2fec..f9b8c5d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.png index d76fdda9..32c39fee 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.png index 8686b255..5439c6b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.png index 3c5739b8..bf6df997 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.png index 51a73200..40e2c9ff 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.png index f0dbeac8..45257270 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.png index c54a0940..ec2b8fd3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.png index cfadb631..e1fa758d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.png index 846af902..5fbbfb79 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.png index 2cac36fa..3056b82c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.png index 17cf32da..04efdd54 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.png index 3c1e1b7f..b63ed40c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.png index 6bfc2a56..f6e6f78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.png index ecf91e12..4072fcb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.png index 050a75a1..94085900 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.png index e3f8a9d9..a6b86b80 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.png index 95ebc0fb..1703efac 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.png index 6e29e9c0..6722a8bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.png index f3aa4f80..28899910 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.png index 1a671a6a..e732acc5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.png index 327e73bb..5476274f 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.png index ad74dda8..95342093 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.png index 6d907e12..000e2b9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.png index 9699ad29..994f2ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.png index 2af6ae5c..25c75afa 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.png index 4dde157f..5382a460 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.png index 4a38d57f..7894a136 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.fits b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.fits index c827df41..1c806b5b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.png index 672900ba..f5ff91c3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png index 6251af88..7caa72d6 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.png index 43be7749..e98b0a62 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.png index a0f7f574..58dba519 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png index 5fc1e693..eb6efa86 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.png index 0af1b7da..1960c6c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/index.html b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/index.html index 0c128261..472b8f6d 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M10.0/index.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.png index 9668f43c..a1070b95 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.png index 75bb6115..f96d245a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.png index 53c634a1..31faee8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.png index 3cbc72c3..958ff385 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.png index 5a974631..c99c2da3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.png index 4bdb3736..9bf18142 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.png index f5e60728..528eb0b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.png index 0dfb26c8..0282952d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.png index 17c57296..1fd48485 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.png index 553e2fec..f9b8c5d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.png index d76fdda9..32c39fee 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.png index 8686b255..5439c6b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.png index 3c5739b8..bf6df997 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.png index 51a73200..40e2c9ff 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.png index f0dbeac8..45257270 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.png index c54a0940..ec2b8fd3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.png index cfadb631..e1fa758d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.png index 846af902..5fbbfb79 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.png index 2cac36fa..3056b82c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.png index 17cf32da..04efdd54 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.png index 3c1e1b7f..b63ed40c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.png index 6bfc2a56..f6e6f78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.png index ecf91e12..4072fcb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.png index 050a75a1..94085900 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.png index e3f8a9d9..a6b86b80 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.png index 95ebc0fb..1703efac 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.png index 6e29e9c0..6722a8bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.png index f3aa4f80..28899910 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.png index 1a671a6a..e732acc5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.png index 327e73bb..5476274f 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.png index ad74dda8..95342093 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.png index 6d907e12..000e2b9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.png index 9699ad29..994f2ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.png index 2af6ae5c..25c75afa 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.png index 4dde157f..5382a460 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.png index 4a38d57f..7894a136 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.fits b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.fits index 811aa324..5a21286a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.png index 251b05b3..4f30b004 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png index 8ef83f2f..6e0e4a6d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.png index 43be7749..e98b0a62 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.png index a0f7f574..58dba519 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png index 5c74f610..94317658 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.png index 0af1b7da..1960c6c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/index.html b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/index.html index 13376dcb..9dfd1779 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M100.0/index.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.png index 9668f43c..a1070b95 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.png index 75bb6115..f96d245a 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.png index 53c634a1..31faee8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.png index 3cbc72c3..958ff385 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.png index 5a974631..c99c2da3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.png index 4bdb3736..9bf18142 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.png index f5e60728..528eb0b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.png index 0dfb26c8..0282952d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.png index 17c57296..1fd48485 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.png index 553e2fec..f9b8c5d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.png index d76fdda9..32c39fee 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.png index 8686b255..5439c6b5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.png index 3c5739b8..bf6df997 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.png index 51a73200..40e2c9ff 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.png index f0dbeac8..45257270 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.png index c54a0940..ec2b8fd3 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.png index cfadb631..e1fa758d 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.png index 846af902..5fbbfb79 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.png index 2cac36fa..3056b82c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.png index 17cf32da..04efdd54 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.png index 3c1e1b7f..b63ed40c 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.png index 6bfc2a56..f6e6f78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.png index ecf91e12..4072fcb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.png index 050a75a1..94085900 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.png index e3f8a9d9..a6b86b80 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.png index 95ebc0fb..1703efac 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.png index 6e29e9c0..6722a8bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.png index f3aa4f80..28899910 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.png index 1a671a6a..e732acc5 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.png index 327e73bb..5476274f 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.png index ad74dda8..95342093 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.png index 6d907e12..000e2b9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.png index 9699ad29..994f2ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.png index 2af6ae5c..25c75afa 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.png index 4dde157f..5382a460 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.png index 4a38d57f..7894a136 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.fits b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.fits index bea0263e..e405ddc7 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.png index 242e941e..1d899ff2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png index 76d862fb..1512845b 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.png index 43be7749..e98b0a62 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.png index a0f7f574..58dba519 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png index b04b3caf..46de7c76 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.png index 0af1b7da..1960c6c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/index.html b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/index.html index 382dc8e0..2ff7d691 100644 --- a/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/index.html +++ b/models/kt2013wd01-25_Z1.0_clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.fits index 7af32f87..f28da548 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.html index b6e69f29..05ef05e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.png index 39ed2807..c12dac4f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.png index f9c8fe70..bf06b18b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.fits index eb4e0f94..96001372 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.html index 9da4c536..7502abcb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.png index 1f24d414..9cef0dae 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.fits index 55f44c23..c4800a65 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.html index 6077b4c3..bd30b013 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.png index d61b6ff9..c9480cd9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.png index 60201ecf..ccde17df 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.png index fc28996d..bf01ec48 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.png index d3903168..935352a5 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.png index 349b5787..22bab411 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.png index 0e987cbb..f87f5082 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.png index 1bd62ecd..a908e8b2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.png index 778b83cf..3e91f310 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.fits index 8d28dd11..ae310c0d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.html index b4dee179..640b77f0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.png index ebc37e86..23d5970b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.fits index 9b18f40f..29862bae 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.html index 06ea2806..a8e2f010 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.png index a23c4b33..72abf250 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.png index 969c0fb0..22c90fcf 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.png index 56c28d47..40c2b990 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.png index 8d216a0d..83307c6f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.fits index e498efb1..8c493688 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.html index fbdf9bf5..3ce17d90 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.png index 48ae82db..39d53c85 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.png index ebc77669..8cd7a456 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.png index 0dec6afd..151ffcd4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.fits index efdc3651..7314758b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.html index 5288f3f1..0d6986c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.png index f84e832a..00d7164a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.png index d86adc47..8fc39fab 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.png index 91894f35..ea5f588e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.fits index 1b4a8776..ac682413 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.html index 5b7503d0..e5ed055d 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.png index 39a2c803..1463e71b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.png index a1021666..557074ae 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.png index 41cafdfa..69062b5b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.fits index 9190df9d..52cd89ea 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.html index 530696f4..85e87d5f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.png index c3e08cd9..a728477e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.png index 2a184cb3..fd9b1f69 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.png index df3934e8..aee3ee0d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.fits index ec988d43..ca23b961 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.html index 65d4cfa5..0cc90e25 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.png index e63df845..8afafb9d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.png index 72490711..cdc64075 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.png index a0b5c21e..4b356f94 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.png index 6fe13a7d..6c199e28 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.fits index 21f8740b..ef60c44a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.html index 13a52f28..534543f3 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.png index e2007769..bb3f2fb4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.png index 701eeb04..416cbb1b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.png index bac02c07..b5aca667 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.fits index d1433f16..86a47629 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.html index 4d11d1c8..8690f288 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.png index 95f8cec0..e8b7d641 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.fits index 29728d5b..2438ee0a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.html index 24278837..8df151af 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.png index 230fa48c..5c4e35f7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.png index e22aafbe..82e79698 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.png index dd937c36..2b2ffcaf 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.png index f941a4cb..8919ee16 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.fits index 0d10f06a..97f7597f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.html index ec79064b..af84022b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.png index 34f563a4..7dec73ce 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.png index 0b254f72..1ec741d8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.png index 4bae0f95..c5265664 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.png index ea2c6a31..535a45a0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.png index 6d67b0c9..e3cc0362 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.png index affc986d..6cb5f2a8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.fits index 8641f070..905c70b4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.html index 5b990171..4ab0ad04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.png index cf247d1b..399f3eb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.png index 9af5cb22..c7d4afe0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.png index 2b5d40a7..d3b20747 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.fits index 58ab03fe..c3398fc3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.html index 2403580f..230a8799 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.png index e5ed47c9..d7ae78d4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.png index 008bfaa8..2937cd86 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.png index 0d649448..e896604a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.fits index b9a42efd..25e57345 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.html index 0460fbbf..f9ae9234 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.png index f23c0889..e11d079c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/CP32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.fits index f1697e3b..8dcb9e57 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.png index ff28069f..a9e031e3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.fits index a0b66121..c99ffd48 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.html index e89e093f..38918936 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.png index a0e5e7b8..c2824d7d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png index c2829807..d35a7ab7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.fits index e70872e6..26c67677 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.html index 793c03b7..c5eabc09 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.png index 0626627e..876bcbe4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.png index 51422077..59d530a8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.png index 31791674..5f074cd9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.fits index 9507be7e..048dfd5d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.html index f2bcd8cf..91980afd 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.png index e41e9203..0b64bc5b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png index d3829929..0b99f2a8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.fits index f7f6b834..5577bec5 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.html index be2fba6b..6e98ae24 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.png index 39110290..3dea2f65 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.png index 23ce75b4..63c9858d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.html index abf8064f..09375cc6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.png index b350d016..a2b12c43 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/Ts.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/index.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/index.html index 4f90e875..b1a02b81 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/index.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.fits index ea55a161..c1d9857d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.html index b6e69f29..05ef05e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.png index 27098763..631b6ee9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.png index e5192607..ff6a1e00 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.fits index 4d760e73..afdca20d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.html index 9da4c536..7502abcb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.png index e8a11d36..24d919c0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.fits index 0c83d870..07734066 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.html index 6077b4c3..bd30b013 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.png index db920ad9..4615524a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.png index e85e7296..c1a60369 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.png index 876a54b0..1b52c94c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.png index 825ceff7..c76f363f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.png index f53c73d1..deb0e198 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.png index 9838c6c0..c4b23521 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.png index f94e066a..135fbb03 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.png index 6dd309dc..0c240396 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.fits index 6c3949a7..baa8d056 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.html index b4dee179..640b77f0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.png index 5d4d85ea..b38232b3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.fits index 8c5724f1..194a3951 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.html index 06ea2806..a8e2f010 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.png index a821cda9..c192460b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.png index f5e14f79..21c6dc16 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.png index 97034e73..42eb006e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.png index d2064169..87431b56 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.fits index 888a97fc..96b734d7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.html index fbdf9bf5..3ce17d90 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.png index d5f00d96..b372f409 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.png index 9cc0dd68..ae721fe2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.png index 0be42d61..920388ef 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.fits index 97b156ab..ba1bb14b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.html index 5288f3f1..0d6986c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.png index 5e875418..64d29025 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.png index d7384db2..fe9a0e51 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.png index 7a790294..ae068751 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.fits index e86fcfb3..9f9ff1ed 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.html index 5b7503d0..e5ed055d 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.png index c1820654..58689350 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.png index 81590f40..9fa1a6c1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.png index 86ff3eb9..5679acb6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.fits index 9ebd9645..aec67935 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.html index 530696f4..85e87d5f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.png index 699bbc27..c5363154 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.png index 7fd61c63..de5c36e8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.png index 50d81131..b019158c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.fits index 3c5672c5..1259ea79 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.html index 65d4cfa5..0cc90e25 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.png index c0e6256c..76c4cc11 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.png index 92388b5c..e060c47b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.png index 56aa60af..d61255dc 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.png index 3ec31d38..28677230 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.fits index 3f5bdc5d..63110f36 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.html index 13a52f28..534543f3 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.png index 12191ea2..2959de55 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.png index a09239b4..126a1aca 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.png index 699730eb..f1d8a2b4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.fits index 49491775..12406a67 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.html index 4d11d1c8..8690f288 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.png index 729cbe1e..8d58bb97 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.fits index 694fe068..090e7766 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.html index 24278837..8df151af 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.png index a90f2be0..ac907596 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.png index bcac21f8..485386fe 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.png index 2a7e3c5c..5bd624c3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.png index 0dbce096..9f3b7af9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.fits index 332f2ff7..eef3e093 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.html index ec79064b..af84022b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.png index 426561a5..371968c4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.png index 9b55a8f9..be587cb0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.png index fada9ca4..8a51f0f0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.png index 727b6b44..bc26b94e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.png index 67581ed9..3015a6fb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.png index e55377fa..d4a0560d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.fits index df8a2df0..8b125e0b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.html index 5b990171..4ab0ad04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.png index 82be9627..ffc2ed90 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.png index caf71def..d124e5b2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.png index 650a13a0..e41ed801 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.fits index 69cc6ba1..a4fe3e90 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.html index 2403580f..230a8799 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.png index 6507afe8..5c21831c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.png index af05c680..b2477d7c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.png index e2ab399d..f606edc0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.fits index 7ae2cf96..9080774b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.html index 0460fbbf..f9ae9234 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.png index 4b4f4150..4bf9281b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/CP32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.fits index 306798d2..a3e2fde6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.png index fcfca894..ce835e1e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.fits index f7dba24e..f38e2461 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.html index e89e093f..38918936 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.png index ed4a50a5..b4524301 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png index 8d5d4e5d..ba28ff7f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.fits index 025092e5..a460a1a9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.html index 793c03b7..c5eabc09 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.png index ecc7f702..1dddf830 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.png index db1ccd99..bea0c59e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.png index 18188eb5..d8497361 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.fits index 090cbfd9..18f6f2f6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.html index f2bcd8cf..91980afd 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.png index ccd6afcd..20a7971e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png index 4f1c5a2a..42280689 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.fits index 56fc8403..70d31076 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.html index be2fba6b..6e98ae24 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.png index efe6d581..9b9e09c2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.png index d4b77855..50ea9661 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.html index abf8064f..09375cc6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.png index f06677ee..8475174a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/Ts.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/index.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/index.html index 2bac0315..0806de04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/index.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.fits index 07734a01..f67566f7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.html index b6e69f29..05ef05e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.png index f8158e56..de6466e9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.png index ccf6ae9e..3a9ecaba 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.fits index af60fd0a..51f088fb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.html index 9da4c536..7502abcb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.png index ff493414..5b6f6522 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.fits index 22006e73..9bf10026 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.html index 6077b4c3..bd30b013 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.png index aa4c0edf..0a07d21a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.png index b584e5ce..aa2d2132 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.png index 6071f44b..75031a91 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.png index 72e2b781..fe0e4388 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.png index 85268cef..06499e7f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.png index 43d2813b..60acea0a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.png index 304f3825..8f343011 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.png index 3635ce92..cee99419 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.fits index 57f20882..2eb0ac53 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.html index b4dee179..640b77f0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.png index f84f8e24..35592142 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.fits index 76c770fa..3b5f5aa0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.html index 06ea2806..a8e2f010 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.png index 5ead078c..c68c37c0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.png index 7e198ab8..2f4a6ad8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.png index 0c69f7a8..4e563c11 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.png index 2b90b958..154ab292 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.fits index 7497c218..e4fb5113 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.html index fbdf9bf5..3ce17d90 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.png index aee05ab1..44184d74 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.png index e0c02089..0eef3805 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.png index 8c4074d7..cc0bf0b3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.fits index 44a9db9b..ae873b32 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.html index 5288f3f1..0d6986c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.png index f48b38ad..7c0c05c3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.png index f037b6ab..7b4b950a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.png index da22adee..8566cbf1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.fits index 547df049..76831a99 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.html index 5b7503d0..e5ed055d 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.png index 5579bbb1..e39ea913 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.png index 084c679b..e8338c3b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.png index 8139b91d..d2d35d9e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.fits index fa53efe7..914ea265 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.html index 530696f4..85e87d5f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.png index 2373ea61..eb455e08 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.png index bd95feaa..1a36a07b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.png index 9f30cde9..9d450f49 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.fits index 2555e6cf..2c8ddaa8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.html index 65d4cfa5..0cc90e25 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.png index 4e5299d9..f72e2347 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.png index f732c97d..6b3245bb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.png index 7d7924e4..6d486534 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.png index e82d33a9..96a4fbe0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.fits index 235afed7..60612c8e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.html index 13a52f28..534543f3 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.png index b47a11ba..f9e93894 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.png index 2ac52e1e..1464af42 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.png index 4b4828df..12cc4162 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.fits index d3cdb7f0..b3f447fa 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.html index 4d11d1c8..8690f288 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.png index a9c52f7b..18c4665e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.fits index f1714865..019a1fcf 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.html index 24278837..8df151af 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.png index 68f6d98f..0b93e97d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.png index d0d7dd83..8df32e2c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.png index 268f7ff9..2fe69baa 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.png index c74e7b7f..83e05d46 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.fits index 2b9a9106..7292c529 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.html index ec79064b..af84022b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.png index beed4fde..f9c3603d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.png index 9a9b98a7..2234dcbd 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.png index 08012af1..d171e92e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.png index ae108d12..56fcbeb9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.png index ef476d9e..d4639be3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.png index d4bba2a4..cbe3ea45 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.fits index e7154233..6c20dc4a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.html index 5b990171..4ab0ad04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.png index 784481a4..8292b735 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.png index 242010b5..57c6fe2f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.png index d4a242c5..07a9506c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.fits index 6a502efb..dbba6929 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.html index 2403580f..230a8799 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.png index 8907bb7c..360db0eb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.png index 3ac8320a..1851453f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.png index e2c6a8ad..35ff9ea1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.fits index 540a8b41..9561ca3c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.html index 0460fbbf..f9ae9234 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.png index 4aebb803..9dd0d695 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/CP32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.fits index 361b9c93..44960eee 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.png index 672900ba..f5ff91c3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.fits index 6a1f6805..f876f61b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.html index e89e093f..38918936 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.png index 22ed7009..59bc9f90 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png index 5697a3ff..9dcfaafd 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.fits index c535da35..649868b6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.html index 793c03b7..c5eabc09 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.png index bf2a14cf..a2a8a513 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.png index a754b619..f35bde87 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.png index c6c23597..c807553f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.fits index 3b1914bd..24517ceb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.html index f2bcd8cf..91980afd 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.png index 8449bc37..aa5fa3ee 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png index 088d127b..48c92e6b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.fits index c743cce2..4b7cf660 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.html index be2fba6b..6e98ae24 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.png index 9168c16d..71ffbced 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.png index 1b3d68c5..f9f69e5f 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.html index abf8064f..09375cc6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.png index f0b7d240..6d08de45 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/Ts.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/index.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/index.html index 1ce80c30..9c2f25ce 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/index.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.fits index 5d100b37..21656261 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.html index b6e69f29..05ef05e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.png index af13a256..a0191697 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.png index ec5773fd..9721a04e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.fits index 40d3c756..dc93d28e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.html index 9da4c536..7502abcb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.png index 082ce6be..184661b6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.fits index 94a3774d..925032f3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.html index 6077b4c3..bd30b013 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.png index 43c89abe..f030ac02 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.png index b255f2eb..3943bec9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.png index 9cde5af1..e84a1abd 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.png index c44f5ad8..945d94da 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.png index 4b0aba21..3f514a23 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.png index 8a7387ab..fc48c256 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.png index f02c21a3..f4c377b0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.png index a9bd6724..1f37aba5 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.fits index f2b29b52..61224883 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.html index b4dee179..640b77f0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.png index 239bde22..28fa2014 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.fits index b7a16069..63393da0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.html index 06ea2806..a8e2f010 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.png index eb513a73..615e25f3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.png index ca8e7a7d..7309ca4e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.png index 3806e4da..51b8c406 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.png index ba8ee33b..202707f3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.fits index 8640e5c7..a7da46db 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.html index fbdf9bf5..3ce17d90 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.png index 3e75a422..78a6a9a9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.png index 28c32e86..ba5ba394 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.png index 420986fb..2f9e4d8a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.fits index b62ceeb8..8c730667 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.html index 5288f3f1..0d6986c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.png index 13007295..66bfbe47 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.png index f29ab982..6b6ed11b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.png index 75364191..db05fd83 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.fits index ebe107bb..4d8ee176 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.html index 5b7503d0..e5ed055d 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.png index e3fe48ba..d6d248fc 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.png index 6a6e82cb..473aa3fb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.png index 1270f80b..4a37db6a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.fits index deabb04e..8912b3cd 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.html index 530696f4..85e87d5f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.png index afac0b62..64d9833e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.png index 8de92d02..ffb0c1a9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.png index b8fad6f4..357f052a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.fits index e986c62b..9cea351d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.html index 65d4cfa5..0cc90e25 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.png index ffc9cc39..1a169486 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.png index 107622e7..66587af0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.png index 9698577a..788257bc 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.png index 8b01c5c0..e082f72c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.fits index efe533cc..c26dce58 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.html index 13a52f28..534543f3 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.png index 23c0b5cf..540f8eab 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.png index d36ddf7b..0ab233ad 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.png index d5547621..55db9d9d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.fits index 2e746697..2c3194c0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.html index 4d11d1c8..8690f288 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.png index 39896bad..e913fa77 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.fits index ea87558d..e2c03b58 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.html index 24278837..8df151af 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.png index 1c68fe75..17914d86 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.png index fb0b8eec..d92dbf85 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.png index d6da4d31..2a7ce940 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.png index 21675f07..7fe29895 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.fits index 1cd7c910..ba928759 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.html index ec79064b..af84022b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.png index 75e77380..bf429758 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.png index 87e5f8ca..1d419c3c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.png index b3288139..956c39be 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.png index 57c4cd65..907d3538 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.png index b2c44841..eb1f61ea 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.png index 99c923b0..c919a933 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.fits index c7625fc6..e6a1f705 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.html index 5b990171..4ab0ad04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.png index 8a405319..e2126b29 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.png index ff281a27..3b2cbf83 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.png index 29eae7e3..66a656fe 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.fits index a41ab942..81b09c16 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.html index 2403580f..230a8799 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.png index 264d9af0..b0eab1d3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.png index bb08887d..d1c30ddf 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.png index af12313a..15c30880 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.fits index be869171..498718d1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.html index 0460fbbf..f9ae9234 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.png index 9bb2ed9f..152099de 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/CP32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.fits index 2ccdfd40..732ca4b9 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.png index 251b05b3..4f30b004 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.fits index 7ac3e93f..82571ada 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.html index e89e093f..38918936 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.png index 40a7a210..27f6b910 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png index f03f9d76..8234ed15 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.fits index c1b5f4f9..355461fc 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.html index 793c03b7..c5eabc09 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.png index 9b7c0c32..aead8786 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.png index 4331f64d..1ae85e7e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.png index 97bd37c9..911620fb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.fits index 911a7bf7..a50b34ca 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.html index f2bcd8cf..91980afd 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.png index 68ba04b7..918e4fea 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png index 6b3f68b6..f6deef70 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.fits index 501e9f16..353b20c4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.html index be2fba6b..6e98ae24 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.png index 442639dc..42c4b305 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.png index 119d3101..05b605fa 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.html index abf8064f..09375cc6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.png index 8725517f..66217d2c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/Ts.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/index.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/index.html index 665d092b..a64a97ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/index.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.fits index fa82e835..57023ced 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.html index b6e69f29..05ef05e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.png index 84ba757c..b729e79b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.html index d3a2833d..3c0c6f66 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.png index 4423404b..54c03681 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.fits index 3afb18fc..3a43660a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.html index 9da4c536..7502abcb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.png index 6dadf123..51bc1447 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.fits index b6455512..71996f8e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.html index 6077b4c3..bd30b013 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.png index b62f2d73..32db4c25 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.html index 4f312b16..9e1a57b0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.png index 6ce4c25d..b01e377d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.html index 1fca1cf1..ce35600e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.png index 8a6f5ff0..85eda030 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.html index 71ecf094..4e08d7a5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.png index 6a3b05db..3d3788cd 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.html index 0273c5ec..81a9ce29 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.png index 6ade2f0d..a600096a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.html index b1b6cea5..02385988 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.png index da54a72c..19426ebe 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.html index 4886eceb..885ed89e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.png index e4e4db0f..553d835a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.html index b7516a36..0a9ddc31 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.png index 75191744..8fb14915 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.fits index b019411d..0666658b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.html index b4dee179..640b77f0 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.png index 2c456b22..ec44d542 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.fits index 5ce60368..7521f4af 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.html index 06ea2806..a8e2f010 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.png index cd534559..b1f4d078 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.html index 419fcce3..03fc2db8 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.png index 872e9928..87efbc15 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.html index 0017854c..d609917e 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.png index 02d34289..b6001170 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.html index 1a9bc16c..ec05738b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.png index 9217ac16..9e2fa48a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.fits index eb20006d..f864a526 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.html index fbdf9bf5..3ce17d90 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.png index d4679f26..0fcc0c72 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html index 89053bbc..bf610903 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png index bef89b42..193b6200 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html index 8013849a..45b5adc1 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png index d7bfc4bf..d67f061e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.fits index 8620d003..7ad27b94 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.html index 5288f3f1..0d6986c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.png index 182c0ebc..9a8d3f84 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html index f110795a..1c8ce32b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png index 1e000cc7..344884a0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html index 870bbe57..f7e6ae1f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png index 8d49b446..eb5358f1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.fits index 18b1391d..b7110b43 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.html index 5b7503d0..e5ed055d 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.png index 78ffccbf..c8222eeb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html index 5f74a1bd..8703c5ad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png index 2ff92a94..98e31ea7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html index a1d6f3d0..342d494f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png index a5cabef1..b12fe1ce 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.fits index 20122f9e..d24d4382 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.html index 530696f4..85e87d5f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.png index ec2322fa..d64c488e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html index d68030c6..abf36091 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png index 9fbc1d24..ced0ead6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html index 71e6e135..8dbb3f01 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png index 5afe683c..b8808538 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.fits index d6c5c71e..a73045ab 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.html index 65d4cfa5..0cc90e25 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.png index c2fa88c6..d872020c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.html index ab803a71..b6d54717 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.png index e2c0a4a2..4de8df24 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.html index 8efa1722..eaeff62f 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.png index 2ea999be..d42bdef4 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.html index 30211668..fa7e7a53 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.png index e70dbab4..968e1061 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.fits index 27bd3ff0..7f2a5842 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.html index 13a52f28..534543f3 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.png index bb87937e..7d8fbbbb 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.html index d4047495..4e2422a6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.png index aaf63eb1..0f0cc380 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.html index 60b3d672..794408c9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.png index 093e3aac..637f2b6e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.fits index 66a03db4..d608cbd8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.html index 4d11d1c8..8690f288 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.png index 941a307b..3de97cd2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.fits index 8cf2b606..140afde5 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.html index 24278837..8df151af 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.png index a3d0c515..c62d88a0 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.html index e130c129..2c056e5c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.png index 431198b1..3dacf900 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.html index 266266c1..6d23ff68 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.png index c5d0b618..014f03a5 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.html index d98cc7ee..bac957fb 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.png index 77574598..7daba733 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.fits index d26d993e..c3ce6cf6 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.html index ec79064b..af84022b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.png index f39fe2d3..9f34a7db 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.html index df327356..457199d5 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.png index b8437986..4762fd6a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.html index 3a8be207..1bf89e3c 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.png index 69582881..78eae014 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.html index 93153f76..dea168ea 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.png index e5ab9e36..cd529d83 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.html index c4f34466..9aa958cc 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.png index b94d631e..c5233310 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.html index c7575b8d..ad873d3b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.png index 480f42f5..e3e7af0a 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.fits index 27c959d6..88533dec 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.html index 5b990171..4ab0ad04 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.png index 648b0c96..407b1e43 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.html index 640edac0..b87733a9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.png index ddaed6c2..e3d4b6a7 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.html index 1b0c5cd4..9823bb51 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.png index e0940436..785f0d7c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.fits index 0219db2f..32bc2aa1 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.html index 2403580f..230a8799 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.png index 1433d131..795990ad 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.html index e0e7858a..269ec22b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.png index 852a07cb..aa22c392 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.html index ec056915..001e8cad 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.png index 90441101..1b2844bf 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.fits index f938c9ab..13b1fa8d 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.html index 0460fbbf..f9ae9234 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.png index a7d6f091..6af012a2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/CP32.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.fits index 545bc84c..5814c773 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.html index 1c683ea4..08556663 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.png index 242e941e..1d899ff2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits index 7090534e..bac83ef8 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.html index e89e093f..38918936 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.png index 39c090a2..3b103b8b 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html index d014d628..008873e9 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png index c8bbb134..3a9aa78e 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.fits index 3f06fd4d..71050d78 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.html index 793c03b7..c5eabc09 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.png index 2dd57bf6..68e41d30 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.html index dacfeb18..0cdc7e28 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.png index 29fb473e..e5abd3f2 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.html index caa4e3fd..2d729fa6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.png index 5216d24f..a49c34a3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits index 7661cf27..af3c9f87 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.html index f2bcd8cf..91980afd 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.png index 3ef53cc4..e1ad9878 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html index d36d7d31..4dafdaac 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png index f95c75f6..2f8a79ed 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.fits b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.fits index ca55a4b3..723c7297 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.fits and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.fits differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.html index be2fba6b..6e98ae24 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.png index 7380b8ac..0fdc2d92 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.html index ae19eeea..cb260c16 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.png index b8c98542..b930ebb3 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.html index abf8064f..09375cc6 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.png b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.png index 73d9aaa1..2650501c 100644 Binary files a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.png and b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/Ts.png differ diff --git a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/index.html b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/index.html index 89fe886d..6e46185b 100644 --- a/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/index.html +++ b/models/kt2013wd01-25_Z1.0_non-clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=5.5, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-25 kt2013wd01-25 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.png index b97404e3..1b75fddc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.png index 1a5b6fbb..632d0c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.png index 4e4e42a2..8975b664 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.png index e73549bc..e5de3f00 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.png index 9bdade5d..069db478 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.png index fc1439c4..8bb2978b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.png index 1632966f..eba9addc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.png index fd18f3c4..1efc7a72 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.png index 8b709111..1db29085 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.png index d73d1556..a983885c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.png index 84dadd53..b3ec3dbd 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.png index 12d845c0..8b60a9bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.png index 635a5c6c..19eff806 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.png index ba80062c..4f963627 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.png index b25dc0de..4e486af1 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.png index 3619696e..03027197 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.png index f2017fd0..fba26662 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.png index 71418172..86ac858c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.png index 3afb7a7f..6a609adc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.png index 303c0ba1..e4e7617e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.png index 2b545fb8..946b17e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.png index d90f536d..bdc0eff9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.png index 86021b61..3c4945ff 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.png index 00c3b359..c6de0942 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.png index a3c7a178..6d805c50 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.png index a07094c2..101c7c4f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.png index e8c92541..46cac95b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.png index 7e5dbc94..b9eeae55 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.png index 676aec40..f262d522 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.png index 4d88ce2c..0f9da8b3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.png index d6037318..773235b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.png index 194ccc30..efeba1ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.png index ffeefd7f..04f79f2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.png index d4d61581..69b23b57 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.png index 5fbd181b..34ccd71d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.png index 58e112a7..fadf7e1e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.fits b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.fits index 673abaf7..7746cb5c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.fits and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.png index 67791f08..537a3ae5 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png index 0fd3c32c..b31710e6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.png index 4ba65429..6c871f70 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.png index 9be25cc2..1680f53b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png index c6261025..8fbd074d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.png index e5aa65a5..bec81a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/index.html b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/index.html index 29386bd2..f509e28f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M0.1/index.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.png index b97404e3..1b75fddc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.png index 1a5b6fbb..632d0c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.png index 4e4e42a2..8975b664 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.png index e73549bc..e5de3f00 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.png index 9bdade5d..069db478 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.png index fc1439c4..8bb2978b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.png index 1632966f..eba9addc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.png index fd18f3c4..1efc7a72 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.png index 8b709111..1db29085 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.png index d73d1556..a983885c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.png index 84dadd53..b3ec3dbd 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.png index 12d845c0..8b60a9bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.png index 635a5c6c..19eff806 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.png index ba80062c..4f963627 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.png index b25dc0de..4e486af1 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.png index 3619696e..03027197 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.png index f2017fd0..fba26662 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.png index 71418172..86ac858c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.png index 3afb7a7f..6a609adc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.png index 303c0ba1..e4e7617e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.png index 2b545fb8..946b17e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.png index d90f536d..bdc0eff9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.png index 86021b61..3c4945ff 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.png index 00c3b359..c6de0942 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.png index a3c7a178..6d805c50 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.png index a07094c2..101c7c4f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.png index e8c92541..46cac95b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.png index 7e5dbc94..b9eeae55 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.png index 676aec40..f262d522 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.png index 4d88ce2c..0f9da8b3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.png index d6037318..773235b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.png index 194ccc30..efeba1ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.png index ffeefd7f..04f79f2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.png index d4d61581..69b23b57 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.png index 5fbd181b..34ccd71d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.png index 58e112a7..fadf7e1e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.fits b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.fits index afa2528d..a2495412 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.png index 25d61a52..0f0fa883 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png index 827039f8..6bf9b15b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.png index 4ba65429..6c871f70 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.png index 9be25cc2..1680f53b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png index 736ae7dc..19df8896 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.png index e5aa65a5..bec81a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/index.html b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/index.html index e33b876a..aa6bdde9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1.0/index.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.png index b97404e3..1b75fddc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.png index 1a5b6fbb..632d0c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.png index 4e4e42a2..8975b664 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.png index e73549bc..e5de3f00 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.png index 9bdade5d..069db478 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.png index fc1439c4..8bb2978b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.png index 1632966f..eba9addc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.png index fd18f3c4..1efc7a72 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.png index 8b709111..1db29085 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.png index d73d1556..a983885c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.png index 84dadd53..b3ec3dbd 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.png index 12d845c0..8b60a9bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.png index 635a5c6c..19eff806 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.png index ba80062c..4f963627 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.png index b25dc0de..4e486af1 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.png index 3619696e..03027197 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.png index f2017fd0..fba26662 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.png index 71418172..86ac858c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.png index 3afb7a7f..6a609adc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.png index 303c0ba1..e4e7617e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.png index 2b545fb8..946b17e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.png index d90f536d..bdc0eff9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.png index 86021b61..3c4945ff 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.png index 00c3b359..c6de0942 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.png index a3c7a178..6d805c50 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.png index a07094c2..101c7c4f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.png index e8c92541..46cac95b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.png index 7e5dbc94..b9eeae55 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.png index 676aec40..f262d522 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.png index 4d88ce2c..0f9da8b3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.png index d6037318..773235b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.png index 194ccc30..efeba1ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.png index ffeefd7f..04f79f2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.png index d4d61581..69b23b57 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.png index 5fbd181b..34ccd71d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.png index 58e112a7..fadf7e1e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.fits b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.fits index d26f2ae7..a954bfd3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.png index 0629b908..4a607010 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png index b48e3355..efee9b7f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.png index 4ba65429..6c871f70 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.png index 9be25cc2..1680f53b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png index 2bfbe2d6..66afe638 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.png index e5aa65a5..bec81a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/index.html b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/index.html index e00ef4df..8da4ed5a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M10.0/index.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.png index b97404e3..1b75fddc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.png index 1a5b6fbb..632d0c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.png index 4e4e42a2..8975b664 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.png index e73549bc..e5de3f00 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.png index 9bdade5d..069db478 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.png index fc1439c4..8bb2978b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.png index 1632966f..eba9addc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.png index fd18f3c4..1efc7a72 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.png index 8b709111..1db29085 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.png index d73d1556..a983885c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.png index 84dadd53..b3ec3dbd 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.png index 12d845c0..8b60a9bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.png index 635a5c6c..19eff806 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.png index ba80062c..4f963627 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.png index b25dc0de..4e486af1 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.png index 3619696e..03027197 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.png index f2017fd0..fba26662 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.png index 71418172..86ac858c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.png index 3afb7a7f..6a609adc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.png index 303c0ba1..e4e7617e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.png index 2b545fb8..946b17e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.png index d90f536d..bdc0eff9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.png index 86021b61..3c4945ff 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.png index 00c3b359..c6de0942 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.png index a3c7a178..6d805c50 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.png index a07094c2..101c7c4f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.png index e8c92541..46cac95b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.png index 7e5dbc94..b9eeae55 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.png index 676aec40..f262d522 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.png index 4d88ce2c..0f9da8b3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.png index d6037318..773235b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.png index 194ccc30..efeba1ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.png index ffeefd7f..04f79f2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.png index d4d61581..69b23b57 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.png index 5fbd181b..34ccd71d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.png index 58e112a7..fadf7e1e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.fits b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.fits index 41c8673f..c02c143b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.png index 544ce9f6..1e7be1a9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png index 8fe67cc2..68b146f2 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.png index 4ba65429..6c871f70 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.png index 9be25cc2..1680f53b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png index e527eb8f..616c0223 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.png index e5aa65a5..bec81a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/index.html b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/index.html index ba528077..a1e8ec31 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M100.0/index.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.png index b97404e3..1b75fddc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.png index 1a5b6fbb..632d0c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.png index 4e4e42a2..8975b664 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.png index e73549bc..e5de3f00 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.png index 9bdade5d..069db478 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.png index fc1439c4..8bb2978b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.png index 1632966f..eba9addc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.png index fd18f3c4..1efc7a72 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.png index 8b709111..1db29085 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.png index d73d1556..a983885c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.png index 84dadd53..b3ec3dbd 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.png index 12d845c0..8b60a9bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.png index 635a5c6c..19eff806 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.png index ba80062c..4f963627 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.png index b25dc0de..4e486af1 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.png index 3619696e..03027197 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.png index f2017fd0..fba26662 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.png index 71418172..86ac858c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.png index 3afb7a7f..6a609adc 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.png index 303c0ba1..e4e7617e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.png index 2b545fb8..946b17e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.png index d90f536d..bdc0eff9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.png index 86021b61..3c4945ff 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.png index 00c3b359..c6de0942 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.png index a3c7a178..6d805c50 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.png index a07094c2..101c7c4f 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.png index e8c92541..46cac95b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.png index 7e5dbc94..b9eeae55 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.png index 676aec40..f262d522 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.png index 4d88ce2c..0f9da8b3 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.png index d6037318..773235b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.png index 194ccc30..efeba1ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.png index ffeefd7f..04f79f2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.png index d4d61581..69b23b57 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.png index 5fbd181b..34ccd71d 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.png index 58e112a7..fadf7e1e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.fits b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.fits index 24fdf8c8..064e40d9 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.png index 2e8a2826..1f71c0b2 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png index ee86fa3e..94f9754c 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.png index 4ba65429..6c871f70 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.png index 9be25cc2..1680f53b 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png index e028443c..4a931300 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.png index e5aa65a5..bec81a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/index.html b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/index.html index 155e80a0..8d326084 100644 --- a/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/index.html +++ b/models/kt2013wd01-7_Z1.0_clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, clumpy, maximum clump mass = 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.fits index f5432316..bc8aafd3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.html index 28bd7da2..24c043e7 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.png index 0229573e..a7cacad7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.png index 4a81d389..c4c0df75 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.fits index 3afe7e92..ec9667e4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.html index 556f3e82..748cc59c 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.png index db061cfa..12589c61 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.fits index 347a5b64..bc25ccc9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.html index b031d1e0..ddb52fbf 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.png index 965a23f7..0db18196 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.png index 8cadf75e..3f5e1aff 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.png index 1cdd2824..cb3189c6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.png index fbea7042..4339ade0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.png index 0367530a..7597c03f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.png index c564ea9c..e0da08a8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.png index 652f1749..9a6a636c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.png index 334faa26..3306a9c0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.fits index e8862cc0..ec9c4d28 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.html index c7e89744..ff27b0c5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.png index a303ebf4..1bf7c974 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.fits index df02544b..8891f17a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.html index ee8a2626..d1173967 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.png index e91aff3d..471ec9cc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.png index 52119f01..a2308ed9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.png index cae93a75..c3f45e22 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.png index 9914bc5f..7a3f9659 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.fits index 25a851a4..5c7a2a64 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.html index 117fe5d0..def2c496 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.png index abfa218a..a4cdeb70 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.png index 9edc0456..56d6ecc5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.png index e32f5148..799e3230 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.fits index 9fb7c275..56196329 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.html index bb6b8ba2..b22955fe 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.png index f72e6fe7..31bbbc8d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.png index 445da5f8..ddd74b5f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.png index 09cbc69a..0676ffeb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.fits index fcddb21d..89b1ac41 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.html index 96a1c9d1..0cb3d1e1 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.png index 58ee38a5..14f75d28 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.png index 4cc70fdc..60c4d296 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.png index 4f7de520..470f7f0d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.fits index 927efabd..38406ee9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.html index 73560a0c..42e4fee9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.png index ada09e5b..1076c200 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.png index 6e8811ee..17d961e3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.png index b7402e07..13deb09d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.fits index d2c2c8be..eaf6ee16 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.html index 02e566ec..d8925497 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.png index c80a9ffe..fc926517 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.png index c5129795..e3fe250d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.png index 5eb1595c..2af70ba3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.png index 783f8b82..8e78639a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.fits index fb45c329..f74ec1fe 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.html index 1b621a81..4ecaa88d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.png index e6969f3a..01c40917 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.png index 8aa776a0..0a19467c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.png index c5009aa5..3b6fea58 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.fits index a69e7d3f..bead9850 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.html index 7d2dbafd..f2a547e2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.png index 400f3375..7e07f083 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.fits index e1eeedbb..603bee67 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.html index 97ade5c3..eb9aef0e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.png index 80318473..9bfb7664 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.png index 5e62796e..9bb68314 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.png index 4780ce09..5eb91952 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.png index 36803ea0..f81c32e8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.fits index 914e9276..01d27fcc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.html index 93beb858..ea156cdc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.png index 5344991b..ec2baa2d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.png index 7af8fb99..87ee3071 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.png index d9025c55..2c70fbc8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.png index e44da986..2275eee0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.png index c2488903..8186d82d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.png index 876929ed..92de3f2b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.fits index 4249c378..f58acfaa 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.html index 66c5216c..553b8d6b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.png index 8072642c..3125b68c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.png index 19a88e20..791c1637 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.png index 97670bd0..68d9e567 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.fits index 6662fd1c..fc608462 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.html index 7dd878ad..7e83b6d2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.png index 77e91c29..1ead7781 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.png index 0ce872fd..ff2275ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.png index ea928a6a..ce116e48 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.fits index be977285..0ee70edd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.html index adfbf901..e59db81f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.png index 68c357e4..e6f9220c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/CP32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.fits index 69c515a7..8e1ba329 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.png index 67791f08..537a3ae5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.fits index b7747aa7..147cc94e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.html index 0229a647..1f3b5cfb 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.png index da31ad8c..bb29375f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png index d9fd8b71..f42cddf4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.fits index 41012bf5..6dc4f51d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.html index 6836abfb..aef20f87 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.png index 8fbc5496..3169ba51 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.png index 14d30a05..c5e030c7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.png index 24b58483..edf44d37 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.fits index e3dd65bc..7d1a5e2c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.html index b0ffb656..ffa8e4be 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.png index e5df6c6e..a8606cee 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png index 9539dded..8ad25a97 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.fits index 81769f35..a30fa868 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.html index 2d608c13..db8bd840 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.png index 56d5fe4e..a9aaef5d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.png index b91a1eaf..a12e8271 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.html index 6aad3746..d2589174 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.png index b350d016..a2b12c43 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/Ts.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/index.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/index.html index 8aefe514..43304ab8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/index.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.fits index b2f928ec..3abdf2ef 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.html index 28bd7da2..24c043e7 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.png index 31c1b659..26b2858a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.png index 388c3708..f544b81e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.fits index 1ae33bc3..6f8a2bbc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.html index 556f3e82..748cc59c 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.png index 08e5f010..a8ff8826 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.fits index d3ed2327..dd23ad12 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.html index b031d1e0..ddb52fbf 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.png index b9eea059..9ed27932 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.png index 2e008e8c..1626c96f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.png index d622ee42..266775e2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.png index 0ac7cb2f..6dfc17ad 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.png index bb7bce1a..c29ff431 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.png index a508ad54..f5b7ea1d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.png index 5fd50369..5e1bc5c3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.png index 8add9a02..7be21c23 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.fits index 114d894e..9ff1aabb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.html index c7e89744..ff27b0c5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.png index 78e1b917..0c5434dd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.fits index c4d1a467..05d9a32c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.html index ee8a2626..d1173967 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.png index 21bba284..5f84eba1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.png index 620fa1a6..5ded29b2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.png index eca7e82e..435705a0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.png index 289c2cd3..b4f33060 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.fits index b7f9ea85..b718fac9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.html index 117fe5d0..def2c496 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.png index ca10523a..2c439489 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.png index 5eb009b4..e8f8aa0a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.png index b00d0ede..30a83415 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.fits index 16567a2e..820f82b0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.html index bb6b8ba2..b22955fe 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.png index fc1ac5c0..a9c3ac01 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.png index 0060fded..7636b44b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.png index 4fe9e859..e924f4af 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.fits index ecffd69a..bc6e9e4e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.html index 96a1c9d1..0cb3d1e1 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.png index a8c95a38..c825f43c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.png index 8eefa823..0268ff03 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.png index 1f86ab49..e0954698 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.fits index 46517ab5..24ba6682 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.html index 73560a0c..42e4fee9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.png index c56ffe49..4822a073 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.png index beb17770..ab271fff 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.png index 2e9a16c6..d1db3181 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.fits index 5bfd6752..9d106cf9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.html index 02e566ec..d8925497 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.png index eef25644..f9f2bb33 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.png index 6327db50..69072e07 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.png index 741017b7..c906447a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.png index 31a121fa..77034167 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.fits index 6f29bc55..e552511e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.html index 1b621a81..4ecaa88d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.png index 6919734f..aef857cc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.png index d8cf39bc..40586a51 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.png index 5460ccbf..0c8378fd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.fits index 329eff66..0d2ff649 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.html index 7d2dbafd..f2a547e2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.png index 70b9b866..d6d1ce10 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.fits index 1d439bb2..d14e6f38 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.html index 97ade5c3..eb9aef0e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.png index 0d098b96..0d5fa31b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.png index d6bbd4f3..cd0c9c01 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.png index 614f3d9a..86d75383 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.png index 9ad2309f..834884b9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.fits index bddd2847..30be94b9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.html index 93beb858..ea156cdc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.png index a14912a2..a9c9dda8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.png index d657fce6..6b1186da 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.png index e69e0a85..aaff8b15 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.png index 01e4f076..93923a13 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.png index f4a8027c..23dd0a84 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.png index a062f48e..5a13fcb2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.fits index b9580b9f..c1b548e9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.html index 66c5216c..553b8d6b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.png index b26cdafb..eac8aea1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.png index fc8537d0..5ec91010 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.png index f77f2682..fe5aa450 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.fits index 16026897..9327b083 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.html index 7dd878ad..7e83b6d2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.png index ebf4ae0a..5ede86cc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.png index 841509bc..f375a992 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.png index dd9dc7f7..559356a2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.fits index aad6b05f..8ac9bede 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.html index adfbf901..e59db81f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.png index 25e3ff00..f158c7ef 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/CP32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.fits index 6e7e0bd2..456258da 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.png index 25d61a52..0f0fa883 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.fits index 6b68cd65..0b2af78a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.html index 0229a647..1f3b5cfb 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.png index 0cfe6280..f481a68a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png index dff92cdd..91489397 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.fits index e71be9ba..36176965 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.html index 6836abfb..aef20f87 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.png index 11d96ede..105e7522 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.png index 20c19411..c3c3d474 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.png index 79d1cae6..3fcdbba5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.fits index 85336b20..a8ebde72 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.html index b0ffb656..ffa8e4be 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.png index 32e0423e..b454688f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png index c30857d1..39828a05 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.fits index a442c62c..71bb6d57 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.html index 2d608c13..db8bd840 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.png index c8400a29..32519985 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.png index 8ca94173..6c2ec699 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.html index 6aad3746..d2589174 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.png index f06677ee..8475174a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/Ts.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/index.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/index.html index 489b370a..8b58e02b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/index.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.fits index 2b839dcc..3f1ecf97 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.html index 28bd7da2..24c043e7 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.png index 7d684175..58453098 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.png index f5918961..36a84807 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.fits index 1ad599b1..f7d906c7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.html index 556f3e82..748cc59c 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.png index 824496f8..47f929bf 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.fits index facea382..68045f61 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.html index b031d1e0..ddb52fbf 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.png index cfc0a90d..036e7415 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.png index c64bc473..29b39ad6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.png index 697b5c6b..939ce1b0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.png index 92850301..1ad4267b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.png index c524b5cb..25bd6bf3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.png index 4282b89a..811288fb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.png index 3d3e3e94..a40943b5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.png index b117fd99..20272986 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.fits index 8c704e06..e88e1886 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.html index c7e89744..ff27b0c5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.png index 4de12b0a..f6bbb41d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.fits index ae2816ac..5f3b77cc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.html index ee8a2626..d1173967 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.png index df3918f3..71c99b28 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.png index 296061dc..aef3c898 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.png index e901ec7d..e2e762e3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.png index a89c5e63..e68a0de0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.fits index 8fbcdcc4..389d7547 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.html index 117fe5d0..def2c496 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.png index 32abc207..78bb70c1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.png index 81ef5c7c..0d735af0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.png index bbd8f93b..27f0e890 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.fits index 4f510916..da02be69 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.html index bb6b8ba2..b22955fe 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.png index e6329a4c..9145a2e5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.png index ae7229ba..691e044c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.png index fd7306c6..203955fe 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.fits index bf582e83..7be58993 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.html index 96a1c9d1..0cb3d1e1 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.png index 28325815..1345f430 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.png index 644db3da..31318bc4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.png index 97b27500..498ef84a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.fits index df780817..f144b4f8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.html index 73560a0c..42e4fee9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.png index da16387d..52985bfc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.png index 8458c886..53436062 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.png index 9cc42fd2..72a6673b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.fits index 296e5947..e481ee4a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.html index 02e566ec..d8925497 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.png index ab59ce86..2081636b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.png index 8e625ce8..fc5dec7d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.png index ff2f2622..08c9749c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.png index 52c55973..068b34f0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.fits index 0f914dec..787c022d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.html index 1b621a81..4ecaa88d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.png index a3eab47e..d9e26c81 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.png index e33ba822..67f372e9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.png index 4196fabf..d683fb56 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.fits index 4a51523e..e1acf6a0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.html index 7d2dbafd..f2a547e2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.png index 56235600..1515f190 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.fits index cea3a1ea..3831963c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.html index 97ade5c3..eb9aef0e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.png index b3990a65..76d56089 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.png index 624a4de5..4dc0f60f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.png index 794a2e25..60d6414e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.png index 5dca5306..dd73ed98 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.fits index 5450dab7..6a4d5f26 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.html index 93beb858..ea156cdc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.png index 1d86d93a..592d87b4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.png index 678dd018..a5056285 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.png index 27749588..fc51a356 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.png index cc0a4443..b1e332db 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.png index 661f3779..a509a60e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.png index 599c0bb0..37c340ee 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.fits index 4452026e..ca3c2ceb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.html index 66c5216c..553b8d6b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.png index d067dfae..039bc69d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.png index 465f44c1..c78c3ef7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.png index 97aa78cd..082e5ab6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.fits index 712b74ec..a3081a85 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.html index 7dd878ad..7e83b6d2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.png index 66221a0b..fe2bcada 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.png index a8f529d7..081b9abc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.png index 006d2650..6c79055c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.fits index 7dc2cb0c..34872621 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.html index adfbf901..e59db81f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.png index ebbfdf98..f559eb39 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/CP32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.fits index d54489d5..dcadba5e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.png index 0629b908..4a607010 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.fits index 0a550e01..4158e258 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.html index 0229a647..1f3b5cfb 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.png index 8ad10f81..b62eecb7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png index 75baed27..1556f3da 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.fits index 82244a61..869b3df1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.html index 6836abfb..aef20f87 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.png index 10980637..d9a1a67a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.png index 2c8fa420..52886ac6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.png index cef6b0fd..05b0beb2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.fits index 114ac1a5..5f80a92c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.html index b0ffb656..ffa8e4be 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.png index f4ef1f3e..8376b2e4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png index 4d890920..6f672817 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.fits index afec172c..bc3fdf34 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.html index 2d608c13..db8bd840 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.png index da9df880..94672467 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.png index da79cab0..9f038ee5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.html index 6aad3746..d2589174 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.png index f0b7d240..6d08de45 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/Ts.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/index.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/index.html index b3dc846e..5e4cd757 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/index.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.fits index 21ec9e2d..794f12ed 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.html index 28bd7da2..24c043e7 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.png index a825a88a..9198a3b6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.png index 8f13b648..f0466c00 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.fits index 4161b5fa..be9fb2c2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.html index 556f3e82..748cc59c 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.png index dd3ddc4f..d252befc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.fits index 207866dc..533d26a1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.html index b031d1e0..ddb52fbf 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.png index bf544fe6..805b0d83 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.png index 16ba684a..6b120ee7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.png index e7faea3b..bb4c162f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.png index cd703502..eddf8c34 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.png index c88c60c4..5c4fbcd8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.png index a87263af..e89df696 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.png index 9ea40891..69fd0371 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.png index 99927d7d..0fd2335a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.fits index a950dd2a..4335e907 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.html index c7e89744..ff27b0c5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.png index 915a782c..645c42c4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.fits index 83797697..ba40091d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.html index ee8a2626..d1173967 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.png index 948e912e..fc09a23c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.png index a14a7b21..c75ebe0c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.png index 05150dd9..3396c27c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.png index ca55ab02..ce67b3db 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.fits index b4740028..d9fea7d4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.html index 117fe5d0..def2c496 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.png index cc3637c4..1e0971ac 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.png index 344cce89..4a227944 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.png index 7f914c82..a078de96 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.fits index fc2e359d..f8d0b193 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.html index bb6b8ba2..b22955fe 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.png index 74a4dd5f..e440b526 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.png index 617de3e3..bd6af49a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.png index c906a694..c0240750 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.fits index 12276562..2e95d964 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.html index 96a1c9d1..0cb3d1e1 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.png index ca3b30c9..f6ca5b4d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.png index 1b2928dd..c8f1d287 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.png index 461be04a..83226cd8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.fits index 0e49bea1..5fd5f725 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.html index 73560a0c..42e4fee9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.png index c4190188..ccf17118 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.png index 210ca661..87b04615 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.png index 493a9b9d..8459862d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.fits index d77d6cb7..0ff3936f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.html index 02e566ec..d8925497 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.png index 319ae516..63fb154f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.png index 442c7098..fc380ce2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.png index 91c85d14..fae7fb9e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.png index 5b7c3918..5aa6df96 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.fits index 62584d0e..c570bb9e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.html index 1b621a81..4ecaa88d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.png index 881c146c..a3d62bfa 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.png index ae2158cf..e1290f68 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.png index 8848559d..915b2395 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.fits index 79ff2c5e..bdc92f24 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.html index 7d2dbafd..f2a547e2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.png index b0988c39..a2ac3dad 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.fits index c3c3a26a..9735542d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.html index 97ade5c3..eb9aef0e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.png index 4ef55677..5c626574 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.png index 1e5a2d70..afe02edc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.png index eb063586..b79560ac 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.png index 5b53e568..582a9a57 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.fits index 23358ef3..5f5c2457 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.html index 93beb858..ea156cdc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.png index db53da9d..b9c95864 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.png index 063a419b..613f1aa8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.png index 17e2f672..8cabd66f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.png index 6670a61e..d0032b79 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.png index 4dd7a514..834316a7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.png index 17369fa1..802f5df6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.fits index d6acfe8e..17df74fe 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.html index 66c5216c..553b8d6b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.png index f5dbfa06..174a92bd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.png index bdfefe7b..ea00bb05 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.png index 14bfe96e..9ca620dd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.fits index b964372b..effb4218 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.html index 7dd878ad..7e83b6d2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.png index 8451db01..8fcf3ea3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.png index 8792b51a..befb52c4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.png index db05d072..e3706470 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.fits index 741341da..02b10f2c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.html index adfbf901..e59db81f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.png index 4128dd6b..33ecd85a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/CP32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.fits index be67d2b2..9417e3e0 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.png index 544ce9f6..1e7be1a9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.fits index 00e72fd3..c51da4ce 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.html index 0229a647..1f3b5cfb 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.png index 2c4fc9a4..17b9ea64 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png index 63cc0598..95554789 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.fits index ad1724e2..520a9817 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.html index 6836abfb..aef20f87 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.png index f7002385..44fa07e1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.png index 612657ea..103bc1a6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.png index ee76a160..e8b415b1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.fits index 9db5d396..b5df2a9d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.html index b0ffb656..ffa8e4be 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.png index 500c6153..81348686 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png index d3450884..2d0dcc1b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.fits index 83dd4076..44ec18fe 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.html index 2d608c13..db8bd840 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.png index 548acf5a..a1c2852d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.png index 1bf16183..25073c62 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.html index 6aad3746..d2589174 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.png index 8725517f..66217d2c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/Ts.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/index.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/index.html index 5b2494a9..1d172235 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/index.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.fits index c83560a9..5a46ad33 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.html index 28bd7da2..24c043e7 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.png index d8ac9186..63eaac35 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.html index 7c8c5f1c..281ddf44 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.png index fe80ff4b..8dba18d7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.fits index 8623f77f..a97ca31e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.html index 556f3e82..748cc59c 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.png index 710a39db..9b570140 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.fits index f8421a82..ab51e4a9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.html index b031d1e0..ddb52fbf 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.png index 5df87f2a..3c322966 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.html index f7a41969..d261494a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.png index 896686b0..ceea3f73 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.html index d165cdb9..98451e9e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.png index e38f8717..a7240199 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.html index 9e66d4d7..afbf7960 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.png index 97c6b40c..5e42f84a 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.html index 6f9aca98..c02d22fc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.png index b504304f..28bdfe8d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.html index aff81193..1a43edf6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.png index 3bf92ec5..73215493 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.html index 94c0eaea..5497f54b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.png index 471bdcf0..d2fda965 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.html index 72fb260e..3b5b6226 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.png index 7c76945e..8424ed6d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.fits index 89d5cc1b..43df3a36 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.html index c7e89744..ff27b0c5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.png index 889452cf..04c87fe7 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.fits index b3199b1a..81c2cd2f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.html index ee8a2626..d1173967 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.png index 6861d2c2..8c095f56 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.html index 0be1971b..23f71600 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.png index bff8bcdb..d002d22c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.html index 0b17e3fb..61a11e5b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.png index f0c9aaab..64d72f43 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.html index 3f1896e4..1c4c4dec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.png index d467ca40..059e471b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.fits index 5f36b29f..ceb187f5 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.html index 117fe5d0..def2c496 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.png index 7d5fea8e..e978e262 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html index d5d97b6c..413e2c27 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png index dac4fd59..a786491c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html index f95f5e2c..127370c4 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png index 0f68aded..c7f8081f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.fits index 6998c6c9..eeb8dc81 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.html index bb6b8ba2..b22955fe 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.png index 2f3bc070..00e72987 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html index 5a3629d4..a7c8fc28 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png index 8c9c0a9c..b4ef69dc 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html index f9b1dcf0..2444f251 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png index 7a8589f0..31d4e62c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.fits index 2c2956d0..da4baed3 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.html index 96a1c9d1..0cb3d1e1 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.png index c5631e7d..778800cb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html index 6a0fbfae..edb230f0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png index 6b54279a..2fee80ca 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html index 5cd95484..4aa220ec 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png index 669600ea..f1f84d65 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.fits index 1def9937..29aaf9cb 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.html index 73560a0c..42e4fee9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.png index 586b8448..39c0f913 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html index 56e1b895..1a3a2a9a 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png index 62092e1d..dd345a7e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html index f673eff1..588d94e5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png index e6438460..d7397a47 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.fits index 6b034d1a..fea44044 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.html index 02e566ec..d8925497 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.png index 3c23b4a6..bcc9fc60 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.html index 506774cb..94e878fa 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.png index 9106669f..a62c329b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.html index feddcd62..2af9e09d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.png index b3e1036c..dc4e8485 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.html index 0c8ef4aa..3ae873e9 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.png index 48159aab..02bfc062 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.fits index f3362ca6..f0f6a98e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.html index 1b621a81..4ecaa88d 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.png index b8d4e865..3a24ba13 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.html index 8fa7a8fb..2afe9f83 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.png index 86c8d818..c970989b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.html index 44c4f1c3..d7de5fc8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.png index e2f63056..451f94db 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.fits index 84dc8ec7..b9c0f8a2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.html index 7d2dbafd..f2a547e2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.png index 994bcb91..6efca6cd 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.fits index 2ee248d4..f3112d48 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.html index 97ade5c3..eb9aef0e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.png index ceea4b63..bbfa89fa 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.html index da1fe1ee..0f505fea 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.png index 40df68f6..d0c10471 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.html index d50e8a8b..f549eef5 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.png index 8cde6d66..5fefcf3e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.html index 537cf650..ad2d18a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.png index 37055ec6..1df11b92 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.fits index b6ba7948..d51e31f4 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.html index 93beb858..ea156cdc 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.png index fe77669e..df9ac5d1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.html index 282d34f3..d86a3068 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.png index e292cf58..e928670f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.html index b508852c..7d686d1f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.png index e5f4bf54..a70fa378 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.html index ac71d56c..c1320012 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.png index 2553e4ca..3e596e7c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.html index 7308477c..db9f1516 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.png index 6d23320e..ccf4fc55 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.html index 64c4b958..cb062da0 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.png index 5fc112a7..b552f505 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.fits index 05cfcf51..e219873e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.html index 66c5216c..553b8d6b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.png index 22a65917..d832898e 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.html index 922d1f04..3cac5a61 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.png index 3bc09da2..58db5e3c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.html index 5a0ac858..fa8b6261 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.png index ad2c6afe..3a819911 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.fits index 93a29b54..0e53d771 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.html index 7dd878ad..7e83b6d2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.png index 0f98f8e0..fa3c358d 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.html index 41cdd881..9c40602b 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.png index d9bb13e9..0f94b9d1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.html index 7a047968..f0934116 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.png index ca549636..76e17399 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.fits index a7f93af4..128c7b5f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.html index adfbf901..e59db81f 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.png index 31f382d7..d0437fe9 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/CP32.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.fits index 5831af49..6f2c0007 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.html index 75990616..a2078fe8 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.png index 2e8a2826..1f71c0b2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits index 94cd7d82..4cfa22ab 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.html index 0229a647..1f3b5cfb 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.png index 3d84b9e3..3f9436e1 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html index ff89181e..2b4b5399 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png index 55fc976a..22806a30 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.fits index a8335b8e..dada79a2 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.html index 6836abfb..aef20f87 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.png index 86c8ad6f..2a1e339b 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.html index ae7cf45b..d3c899d6 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.png index 53b465fa..4dd0850f 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.html index 23a10888..3d899674 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.png index 96d898ac..e08c3488 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits index 83dc1a77..1393acca 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.html index b0ffb656..ffa8e4be 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.png index f9f163f6..92f64fae 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html index d038ab68..d6bfbdb2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png index 65d19e6d..d3fb3fb6 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.fits b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.fits index 52027d79..b0e354a8 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.fits and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.fits differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.html index 2d608c13..db8bd840 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.png index 227bbf99..6b63e850 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.html index bf52156e..aefe385e 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.png index 3fbca175..dc1cc1cf 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.html index 6aad3746..d2589174 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2013 PDR code. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.png b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.png index 73d9aaa1..2650501c 100644 Binary files a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.png and b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/Ts.png differ diff --git a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/index.html b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/index.html index 939b7a1e..b833f5a2 100644 --- a/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/index.html +++ b/models/kt2013wd01-7_Z1.0_non-clumpy_M1000.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0

+KOSMA-tau 2013 models, Weingarter & Draine 2001 RV=3.1, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2013wd01-7 kt2013wd01-7 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2013 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CI370.fits b/models/kt2020_Z1.0_clumpy_M0.0/CI370.fits deleted file mode 100644 index aeea2e30..00000000 Binary files a/models/kt2020_Z1.0_clumpy_M0.0/CI370.fits and /dev/null differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CI370.html b/models/kt2020_Z1.0_clumpy_M0.0/CI370.html deleted file mode 100644 index 6415713a..00000000 --- a/models/kt2020_Z1.0_clumpy_M0.0/CI370.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
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-[C I] 370 µm Intensity -

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-[C I] 370 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C I] 370 µm/[C I] 609 µm Intensity Ratio -

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-[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C I] 609 µm Intensity -

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-[C I] 609 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm Intensity -

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-[C II] 158 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/[C I] 609 µm Intensity Ratio -

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-[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=1-0) Intensity Ratio -

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-[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=2-1) Intensity Ratio -

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-[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=3-2) Intensity Ratio -

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-[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=4-3) Intensity Ratio -

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-[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=5-4) Intensity Ratio -

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-[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[C II] 158 µm/CO(J=6-5) Intensity Ratio -

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-[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=1-0) Intensity -

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-CO(J=1-0) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=10-9) Intensity -

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-CO(J=10-9) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=10-9)/CO(J=5-4) Intensity Ratio -

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-CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=10-9)/CO(J=6-5) Intensity Ratio -

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-CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=10-9)/CO(J=7-6) Intensity Ratio -

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-CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-CO(J=11-10) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=11-10)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=11-10)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=12-11) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=12-11) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=12-11)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=12-11)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=13-12) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=13-12) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=13-12)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=13-12)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=14-13) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=14-13) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=14-13)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=14-13)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=2-1) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=2-1) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=2-1)/CO(J=1-0) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=3-2) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=3-2) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=3-2)/CO(J=1-0) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=3-2)/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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- - CO(J=3-2)/CO(J=2-1) Intensity Ratio - -
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-CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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pdrtpy ModelSet: kt2020

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-CO(J=4-3) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=4-3)/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=5-4) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=5-4) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=4-3) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=9-8) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-The FITS file is available for download. -

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-The FITS file is available for download. -

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-IFIR -

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-The FITS file is available for download. -

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-[O I] 145 µm + [C II] 158 µm Intensity -

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-[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio -

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-[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 145 µm Intensity -

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-[O I] 145 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 63 µm + [C II] 158 µm Intensity -

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pdrtpy ModelSet: kt2020

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-[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 63 µm Intensity -

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pdrtpy ModelSet: kt2020

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-[O I] 63 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 63 µm/[C II] 158 µm Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0

-

-Below are links to the individual FITS files -and plots in the kt2020 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. - -

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[C I] 609 µm Intensity[C I] 370 µm Intensity[O I] 63 µm Intensity[O I] 145 µm Intensity
[C II] 158 µm IntensityCO(J=1-0) IntensityCO(J=2-1) IntensityCO(J=3-2) Intensity
CO(J=4-3) IntensityCO(J=5-4) IntensityCO(J=6-5) IntensityCO(J=7-6) Intensity
CO(J=8-7) IntensityCO(J=9-8) IntensityCO(J=10-9) IntensityCO(J=11-10) Intensity
CO(J=12-11) IntensityCO(J=13-12) IntensityCO(J=14-13) IntensityIFIR
[O I] 63 µm + [C II] 158 µm Intensity[O I] 145 µm + [C II] 158 µm Intensity[O I] 145 µm/[O I] 63 µm Intensity Ratio[O I] 145 µm/[C II] 158 µm Intensity Ratio
[O I] 63 µm/[C II] 158 µm Intensity Ratio[C II] 158 µm/[C I] 609 µm Intensity Ratio[C I] 370 µm/[C I] 609 µm Intensity Ratio[C II] 158 µm/CO(J=1-0) Intensity Ratio
[C II] 158 µm/CO(J=2-1) Intensity Ratio[C II] 158 µm/CO(J=3-2) Intensity Ratio[C II] 158 µm/CO(J=4-3) Intensity Ratio[C II] 158 µm/CO(J=5-4) Intensity Ratio
[C II] 158 µm/CO(J=6-5) Intensity RatioCO(J=2-1)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=2-1) Intensity Ratio
CO(J=4-3)/CO(J=1-0) Intensity RatioCO(J=4-3)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=1-0) Intensity RatioCO(J=6-5)/CO(J=2-1) Intensity Ratio
CO(J=6-5)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=1-0) Intensity RatioCO(J=7-6)/CO(J=2-1) Intensity RatioCO(J=7-6)/CO(J=4-3) Intensity Ratio
CO(J=7-6)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=6-5) Intensity RatioCO(J=8-7)/CO(J=5-4) Intensity RatioCO(J=8-7)/CO(J=6-5) Intensity Ratio
CO(J=9-8)/CO(J=5-4) Intensity RatioCO(J=9-8)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=5-4) Intensity RatioCO(J=10-9)/CO(J=6-5) Intensity Ratio
CO(J=10-9)/CO(J=7-6) Intensity RatioCO(J=11-10)/CO(J=5-4) Intensity RatioCO(J=11-10)/CO(J=6-5) Intensity RatioCO(J=12-11)/CO(J=5-4) Intensity Ratio
CO(J=12-11)/CO(J=6-5) Intensity RatioCO(J=13-12)/CO(J=5-4) Intensity RatioCO(J=13-12)/CO(J=6-5) Intensity RatioCO(J=14-13)/CO(J=5-4) Intensity Ratio
CO(J=14-13)/CO(J=6-5) Intensity Ratio[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio
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- - - - - diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI370.fits b/models/kt2020_Z1.0_clumpy_M0.1/CI370.fits index 99001c41..34c96cb6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CI370.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CI370.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI370.html b/models/kt2020_Z1.0_clumpy_M0.1/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CI370.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI370.png b/models/kt2020_Z1.0_clumpy_M0.1/CI370.png index 55ef5068..ef24cd39 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CI370.png and b/models/kt2020_Z1.0_clumpy_M0.1/CI370.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.html b/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.png b/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.png index 4f44e6d4..8c09d1a1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.png and b/models/kt2020_Z1.0_clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI609.fits b/models/kt2020_Z1.0_clumpy_M0.1/CI609.fits index 28098de2..3e92b64e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CI609.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CI609.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI609.html b/models/kt2020_Z1.0_clumpy_M0.1/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CI609.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CI609.png b/models/kt2020_Z1.0_clumpy_M0.1/CI609.png index 7cdb0ab6..1f1f170d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CI609.png and b/models/kt2020_Z1.0_clumpy_M0.1/CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158.fits b/models/kt2020_Z1.0_clumpy_M0.1/CII158.fits index e7137998..d654f2cd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158.png index 1ebb1844..1d94a8d6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.png index 3db7a0a6..22eaf152 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.png index 76f0e29a..88ed24d5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.png index 4602bdb9..b9cada98 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.png index 71b4385c..22c2815a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.png index 3f1ebd01..ba3a8eb9 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.png index 94627fb1..e7b6419b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.png index 8686eac3..5f7f360b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO10.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO10.fits index 49535473..47cda8ba 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO10.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO10.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO10.png index a07a72df..4976b3a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO109.fits index 9da560b1..f64b84a2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO109.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO109.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109.html b/models/kt2020_Z1.0_clumpy_M0.1/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO109.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109.png b/models/kt2020_Z1.0_clumpy_M0.1/CO109.png index 1b1d5b6a..8b542cc8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO109.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO109.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.png index 91b30060..6333cb10 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.png index 4657a346..c15a9d05 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.html b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.png b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.png index 1f505052..1229b006 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.fits index 5a3010d3..85ef1952 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.png index 3565fa9d..21b4e992 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1110.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1110.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.png index 299d8d63..a9c03943 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.png index a01cf53b..c727e7af 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.fits index 86ae2c8c..307a3107 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.png index 91424eae..90697514 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1211.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1211.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.png index 7c3f8e70..bd4e86e3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.png index ac88775b..21143410 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.fits index 255152ba..6e1ac902 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.png index 7f153e47..b97b1e69 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1312.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1312.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.png index bc895751..d5fb4c12 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.png index ff3e56a7..77011d29 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.fits index 388ee383..72b34386 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.png index f006a7b7..cb08db1c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1413.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1413.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.png index aed89cba..70f493c8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.png index cc9e676d..19ff42f2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO21.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO21.fits index e4205555..cb93ba21 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO21.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO21.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CO21.png index 94c1b9b5..2717ce9e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.png index 7e7b7c71..e0b87386 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO32.fits index ddeb6957..27014048 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO32.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO32.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32.html b/models/kt2020_Z1.0_clumpy_M0.1/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO32.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32.png b/models/kt2020_Z1.0_clumpy_M0.1/CO32.png index 53a02ebd..38d3f149 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO32.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.png index 33a2e1a5..2296c7bf 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.png index 73932dbd..a880bf7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO43.fits index b92ad7f4..552b485a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO43.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO43.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43.html b/models/kt2020_Z1.0_clumpy_M0.1/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO43.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43.png b/models/kt2020_Z1.0_clumpy_M0.1/CO43.png index e1dd4f99..d437fadd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO43.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.png index 6fce2242..86ff8df3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.png index 23071d1c..0d131e9d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO54.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO54.fits index 548be609..74778bc9 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO54.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO54.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO54.png index e67feb75..7ad345d1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO65.fits index 6dec81a8..16fea36e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO65.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO65.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO65.png index 25ff0be8..104e20ea 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.png index 6c63dc93..e74853b8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.png index 8a48b36d..b06e6607 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.png index 148b90aa..29b88d6f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO76.fits index 758c602b..b3e5ce29 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO76.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76.png index 3af760f9..2a68505f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.png index 8689cd49..661a25ae 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.png index 12d68930..77f23b8e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.png index 7eefea87..4366577d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.png index e5c517f9..5c75ed7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.png index 82ce487e..8040b88d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO87.fits index d45e531d..40fc5bcc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO87.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO87.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87.html b/models/kt2020_Z1.0_clumpy_M0.1/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO87.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87.png b/models/kt2020_Z1.0_clumpy_M0.1/CO87.png index f3623e11..a3767e04 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO87.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO87.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.png index dd34a4d3..445e8bef 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.png index 5b349b58..e3c5ca9f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98.fits b/models/kt2020_Z1.0_clumpy_M0.1/CO98.fits index 36de0dd6..2e806ed2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO98.fits and b/models/kt2020_Z1.0_clumpy_M0.1/CO98.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98.html b/models/kt2020_Z1.0_clumpy_M0.1/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO98.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98.png b/models/kt2020_Z1.0_clumpy_M0.1/CO98.png index 7889d4cc..dd270e31 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO98.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO98.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.html b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.png b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.png index 60283c5f..a95806db 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.html b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.png b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.png index 433aae98..ebdb92a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.png and b/models/kt2020_Z1.0_clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/FIR.fits b/models/kt2020_Z1.0_clumpy_M0.1/FIR.fits index 9468f05b..65356ba0 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/FIR.fits and b/models/kt2020_Z1.0_clumpy_M0.1/FIR.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/FIR.html b/models/kt2020_Z1.0_clumpy_M0.1/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/FIR.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/FIR.png b/models/kt2020_Z1.0_clumpy_M0.1/FIR.png index 3b60aeab..29ed0f6e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/FIR.png and b/models/kt2020_Z1.0_clumpy_M0.1/FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.fits b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.fits index 74ccae67..0055a6ec 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.fits and b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.html b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.png b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.png index 23182696..05cc7558 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png index a07bcba0..13c0fd67 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145.fits b/models/kt2020_Z1.0_clumpy_M0.1/OI145.fits index 9c8fae4f..79aa1f32 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145.fits and b/models/kt2020_Z1.0_clumpy_M0.1/OI145.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145.html b/models/kt2020_Z1.0_clumpy_M0.1/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI145.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145.png b/models/kt2020_Z1.0_clumpy_M0.1/OI145.png index a6f3d7ca..5c24e623 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI145.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.html b/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.png b/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.png index 9e0ac30e..fd6cee7f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.html b/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.png b/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.png index 1b4d9752..b1f3c7ab 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.fits b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.fits index 51bf46ae..2ddd3d86 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.fits and b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.html b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.png b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.png index 274f9f1a..4f3bb0cc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png index dc655b50..7116fa4e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63.fits b/models/kt2020_Z1.0_clumpy_M0.1/OI63.fits index 8a651f2d..add24363 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63.fits and b/models/kt2020_Z1.0_clumpy_M0.1/OI63.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63.html b/models/kt2020_Z1.0_clumpy_M0.1/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI63.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63.png b/models/kt2020_Z1.0_clumpy_M0.1/OI63.png index 5f98af81..c0b7cc47 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.html b/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.png b/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.png index 4685f53e..bea313e6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.png and b/models/kt2020_Z1.0_clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.1/index.html b/models/kt2020_Z1.0_clumpy_M0.1/index.html index 2dbbf456..14694e64 100644 --- a/models/kt2020_Z1.0_clumpy_M0.1/index.html +++ b/models/kt2020_Z1.0_clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI370.fits b/models/kt2020_Z1.0_clumpy_M1.0/CI370.fits index c0f81c9b..ef88fbd6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CI370.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI370.html b/models/kt2020_Z1.0_clumpy_M1.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CI370.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI370.png b/models/kt2020_Z1.0_clumpy_M1.0/CI370.png index 55ef5068..ef24cd39 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CI370.png and b/models/kt2020_Z1.0_clumpy_M1.0/CI370.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.html b/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.png b/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.png index 4f44e6d4..8c09d1a1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.png and b/models/kt2020_Z1.0_clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI609.fits b/models/kt2020_Z1.0_clumpy_M1.0/CI609.fits index e9c06fb7..8548a1e6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CI609.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI609.html b/models/kt2020_Z1.0_clumpy_M1.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CI609.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CI609.png b/models/kt2020_Z1.0_clumpy_M1.0/CI609.png index 7cdb0ab6..1f1f170d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CI609.png and b/models/kt2020_Z1.0_clumpy_M1.0/CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158.fits b/models/kt2020_Z1.0_clumpy_M1.0/CII158.fits index 3f33577c..8be2b91e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158.png index 1ebb1844..1d94a8d6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.png index 3db7a0a6..22eaf152 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.png index 76f0e29a..88ed24d5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.png index 4602bdb9..b9cada98 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.png index 71b4385c..22c2815a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.png index 3f1ebd01..ba3a8eb9 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.png index 94627fb1..e7b6419b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.png index 8686eac3..5f7f360b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO10.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO10.fits index a327f47c..94511f00 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO10.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO10.png index a07a72df..4976b3a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO109.fits index 01ff1b87..39532690 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO109.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109.html b/models/kt2020_Z1.0_clumpy_M1.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO109.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109.png b/models/kt2020_Z1.0_clumpy_M1.0/CO109.png index 1b1d5b6a..8b542cc8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO109.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO109.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.png index 91b30060..6333cb10 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.png index 4657a346..c15a9d05 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.html b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.png b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.png index 1f505052..1229b006 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.fits index 80a3d7f0..d97874ee 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.png index 3565fa9d..21b4e992 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1110.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.png index 299d8d63..a9c03943 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.png index a01cf53b..c727e7af 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.fits index 17633f29..6b7e7a57 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.png index 91424eae..90697514 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1211.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.png index 7c3f8e70..b6b129ae 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.png index ac88775b..21143410 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.fits index 1b1e3ddf..84f1b2a2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.png index 7f153e47..b97b1e69 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1312.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.png index bc895751..d5fb4c12 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.png index ff3e56a7..77011d29 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.fits index 6bd22067..0b85e483 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.png index f006a7b7..cb08db1c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1413.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.png index aed89cba..70f493c8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.png index cc9e676d..19ff42f2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO21.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO21.fits index ae1a0665..ee7a242a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO21.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CO21.png index 94c1b9b5..2717ce9e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.png index 7e7b7c71..e0b87386 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO32.fits index 614e4ec0..f9874c14 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO32.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32.html b/models/kt2020_Z1.0_clumpy_M1.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO32.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32.png b/models/kt2020_Z1.0_clumpy_M1.0/CO32.png index 53a02ebd..38d3f149 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO32.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.png index 33a2e1a5..2296c7bf 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.png index 73932dbd..a880bf7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO43.fits index 9eb9a841..5657859b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO43.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43.html b/models/kt2020_Z1.0_clumpy_M1.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO43.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43.png b/models/kt2020_Z1.0_clumpy_M1.0/CO43.png index e1dd4f99..d437fadd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO43.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.png index 6fce2242..86ff8df3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.png index 23071d1c..0d131e9d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO54.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO54.fits index 71c2267a..da9da1ba 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO54.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO54.png index e67feb75..7ad345d1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO65.fits index 5bad29ef..54a4d00a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO65.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO65.png index 25ff0be8..104e20ea 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.png index 6c63dc93..e74853b8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.png index 8a48b36d..4acb6dc7 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.png index 148b90aa..e7a27489 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO76.fits index 8ab98afc..13264a69 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76.png index 3af760f9..2a68505f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.png index 8689cd49..661a25ae 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.png index 12d68930..77f23b8e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.png index 7eefea87..4366577d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.png index e5c517f9..a1aee361 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.png index 82ce487e..8040b88d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO87.fits index eb28990b..ca5b3c50 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO87.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87.html b/models/kt2020_Z1.0_clumpy_M1.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO87.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87.png b/models/kt2020_Z1.0_clumpy_M1.0/CO87.png index f3623e11..a3767e04 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO87.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO87.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.png index dd34a4d3..445e8bef 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.png index 5b349b58..e3c5ca9f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98.fits b/models/kt2020_Z1.0_clumpy_M1.0/CO98.fits index 553f1873..1b2f1e64 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO98.fits and b/models/kt2020_Z1.0_clumpy_M1.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98.html b/models/kt2020_Z1.0_clumpy_M1.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO98.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98.png b/models/kt2020_Z1.0_clumpy_M1.0/CO98.png index 7889d4cc..dd270e31 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO98.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO98.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.html b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.png b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.png index 60283c5f..a95806db 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.html b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.png b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.png index 433aae98..ebdb92a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.png and b/models/kt2020_Z1.0_clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/FIR.fits b/models/kt2020_Z1.0_clumpy_M1.0/FIR.fits index 3ce972fb..3e3864ab 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/FIR.fits and b/models/kt2020_Z1.0_clumpy_M1.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/FIR.html b/models/kt2020_Z1.0_clumpy_M1.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/FIR.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/FIR.png b/models/kt2020_Z1.0_clumpy_M1.0/FIR.png index 0af76e75..a101f086 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/FIR.png and b/models/kt2020_Z1.0_clumpy_M1.0/FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.fits b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.fits index 5c37850f..eb136122 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.fits and b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.html b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.png b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.png index 23182696..05cc7558 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png index 80d654fe..0d4150a2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145.fits b/models/kt2020_Z1.0_clumpy_M1.0/OI145.fits index 45a17905..7f0a3eb6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145.fits and b/models/kt2020_Z1.0_clumpy_M1.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145.html b/models/kt2020_Z1.0_clumpy_M1.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI145.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145.png b/models/kt2020_Z1.0_clumpy_M1.0/OI145.png index a6f3d7ca..5c24e623 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI145.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.html b/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.png b/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.png index 9e0ac30e..fd6cee7f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.html b/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.png b/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.png index 1b4d9752..b1f3c7ab 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.fits b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.fits index fa8900a9..154afc94 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.fits and b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.html b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.png b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.png index 274f9f1a..4f3bb0cc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png index bffef1f1..256a565c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63.fits b/models/kt2020_Z1.0_clumpy_M1.0/OI63.fits index 603e5d92..26e3bd41 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63.fits and b/models/kt2020_Z1.0_clumpy_M1.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63.html b/models/kt2020_Z1.0_clumpy_M1.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI63.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63.png b/models/kt2020_Z1.0_clumpy_M1.0/OI63.png index 5f98af81..c0b7cc47 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.html b/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.png b/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.png index 4685f53e..bea313e6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.png and b/models/kt2020_Z1.0_clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1.0/index.html b/models/kt2020_Z1.0_clumpy_M1.0/index.html index df75eec8..0b4dc244 100644 --- a/models/kt2020_Z1.0_clumpy_M1.0/index.html +++ b/models/kt2020_Z1.0_clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI370.fits b/models/kt2020_Z1.0_clumpy_M10.0/CI370.fits index 3b5d897f..51346080 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CI370.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI370.html b/models/kt2020_Z1.0_clumpy_M10.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CI370.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI370.png b/models/kt2020_Z1.0_clumpy_M10.0/CI370.png index 55ef5068..ef24cd39 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CI370.png and b/models/kt2020_Z1.0_clumpy_M10.0/CI370.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.html b/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.png b/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.png index 4f44e6d4..8c09d1a1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.png and b/models/kt2020_Z1.0_clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI609.fits b/models/kt2020_Z1.0_clumpy_M10.0/CI609.fits index d3957a5f..e0096fbd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CI609.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI609.html b/models/kt2020_Z1.0_clumpy_M10.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CI609.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CI609.png b/models/kt2020_Z1.0_clumpy_M10.0/CI609.png index 7cdb0ab6..1f1f170d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CI609.png and b/models/kt2020_Z1.0_clumpy_M10.0/CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158.fits b/models/kt2020_Z1.0_clumpy_M10.0/CII158.fits index 8762b8a1..8b11d535 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158.png index 1ebb1844..1d94a8d6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.png index 3db7a0a6..22eaf152 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.png index 76f0e29a..88ed24d5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.png index 4602bdb9..b9cada98 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.png index 71b4385c..22c2815a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.png index 3f1ebd01..ba3a8eb9 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.png index 94627fb1..e7b6419b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.png index 8686eac3..5f7f360b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO10.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO10.fits index 75fd1c89..bc3433d4 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO10.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO10.png index a07a72df..4976b3a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO109.fits index 3dcdfb11..d3fd714f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO109.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109.html b/models/kt2020_Z1.0_clumpy_M10.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO109.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109.png b/models/kt2020_Z1.0_clumpy_M10.0/CO109.png index 1b1d5b6a..8b542cc8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO109.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO109.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.png index 91b30060..6333cb10 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.png index 4657a346..c15a9d05 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.html b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.png b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.png index 1f505052..1229b006 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.fits index 23f1bd3d..9e3684c8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.png index 3565fa9d..21b4e992 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1110.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.png index 299d8d63..a9c03943 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.png index a01cf53b..c727e7af 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.fits index 43577d92..8a6342aa 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.png index 91424eae..90697514 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1211.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.png index 7c3f8e70..bd4e86e3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.png index ac88775b..21143410 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.fits index 8976e268..1ff39952 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.png index 7f153e47..b97b1e69 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1312.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.png index bc895751..d5fb4c12 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.png index ff3e56a7..77011d29 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.fits index 28bcbcd5..986ca0a2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.png index f006a7b7..cb08db1c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1413.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.png index aed89cba..70f493c8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.png index cc9e676d..19ff42f2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO21.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO21.fits index 4cba3677..2d4ac59b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO21.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CO21.png index 94c1b9b5..2717ce9e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.png index 7e7b7c71..e0b87386 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO32.fits index b9fddd46..fa665970 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO32.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32.html b/models/kt2020_Z1.0_clumpy_M10.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO32.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32.png b/models/kt2020_Z1.0_clumpy_M10.0/CO32.png index 53a02ebd..38d3f149 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO32.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.png index 33a2e1a5..2296c7bf 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.png index 73932dbd..a880bf7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO43.fits index 5cdbbe77..154f7b34 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO43.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43.html b/models/kt2020_Z1.0_clumpy_M10.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO43.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43.png b/models/kt2020_Z1.0_clumpy_M10.0/CO43.png index e1dd4f99..d437fadd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO43.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.png index 6fce2242..86ff8df3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.png index 23071d1c..0d131e9d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO54.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO54.fits index 3587d64d..a505cf93 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO54.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO54.png index e67feb75..7ad345d1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO65.fits index 08c82562..39532217 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO65.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO65.png index 25ff0be8..104e20ea 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.png index 6c63dc93..e74853b8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.png index 8a48b36d..b06e6607 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.png index 148b90aa..29b88d6f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO76.fits index 71d9d0df..0fb2cb0c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76.png index 3af760f9..2a68505f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.png index 8689cd49..661a25ae 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.png index 12d68930..77f23b8e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.png index 7eefea87..4366577d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.png index e5c517f9..5c75ed7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.png index 82ce487e..8040b88d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO87.fits index b9c46fc2..70baa26a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO87.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87.html b/models/kt2020_Z1.0_clumpy_M10.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO87.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87.png b/models/kt2020_Z1.0_clumpy_M10.0/CO87.png index f3623e11..a3767e04 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO87.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO87.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.png index dd34a4d3..445e8bef 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.png index 5b349b58..57871a90 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98.fits b/models/kt2020_Z1.0_clumpy_M10.0/CO98.fits index d8e41a92..5a5c61c2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO98.fits and b/models/kt2020_Z1.0_clumpy_M10.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98.html b/models/kt2020_Z1.0_clumpy_M10.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO98.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98.png b/models/kt2020_Z1.0_clumpy_M10.0/CO98.png index 7889d4cc..dd270e31 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO98.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO98.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.html b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.png b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.png index 60283c5f..a95806db 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.html b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.png b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.png index 433aae98..ebdb92a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.png and b/models/kt2020_Z1.0_clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/FIR.fits b/models/kt2020_Z1.0_clumpy_M10.0/FIR.fits index f953e539..70671cde 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/FIR.fits and b/models/kt2020_Z1.0_clumpy_M10.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/FIR.html b/models/kt2020_Z1.0_clumpy_M10.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/FIR.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/FIR.png b/models/kt2020_Z1.0_clumpy_M10.0/FIR.png index c6c69b44..2dedb80a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/FIR.png and b/models/kt2020_Z1.0_clumpy_M10.0/FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.fits b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.fits index 07471fd0..c796bfb5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.fits and b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.html b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.png b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.png index 23182696..05cc7558 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png index e4288a2c..802c370a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145.fits b/models/kt2020_Z1.0_clumpy_M10.0/OI145.fits index 94a789ac..c92a911b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145.fits and b/models/kt2020_Z1.0_clumpy_M10.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145.html b/models/kt2020_Z1.0_clumpy_M10.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI145.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145.png b/models/kt2020_Z1.0_clumpy_M10.0/OI145.png index a6f3d7ca..5c24e623 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI145.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.html b/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.png b/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.png index 9e0ac30e..fd6cee7f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.html b/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.png b/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.png index 1b4d9752..b1f3c7ab 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.fits b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.fits index e3d7f0c8..8aa3cf61 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.fits and b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.html b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.png b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.png index 274f9f1a..4f3bb0cc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png index 9f20617a..8402c7c6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63.fits b/models/kt2020_Z1.0_clumpy_M10.0/OI63.fits index 5ce9e455..cbaa97f7 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63.fits and b/models/kt2020_Z1.0_clumpy_M10.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63.html b/models/kt2020_Z1.0_clumpy_M10.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI63.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63.png b/models/kt2020_Z1.0_clumpy_M10.0/OI63.png index 5f98af81..c0b7cc47 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.html b/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.png b/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.png index 4685f53e..bea313e6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.png and b/models/kt2020_Z1.0_clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M10.0/index.html b/models/kt2020_Z1.0_clumpy_M10.0/index.html index 2408f879..dce00eaf 100644 --- a/models/kt2020_Z1.0_clumpy_M10.0/index.html +++ b/models/kt2020_Z1.0_clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI370.fits b/models/kt2020_Z1.0_clumpy_M100.0/CI370.fits index c438f3f0..fc1990b8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CI370.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI370.html b/models/kt2020_Z1.0_clumpy_M100.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CI370.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI370.png b/models/kt2020_Z1.0_clumpy_M100.0/CI370.png index 55ef5068..ef24cd39 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CI370.png and b/models/kt2020_Z1.0_clumpy_M100.0/CI370.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.html b/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.png b/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.png index 4f44e6d4..8c09d1a1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.png and b/models/kt2020_Z1.0_clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI609.fits b/models/kt2020_Z1.0_clumpy_M100.0/CI609.fits index 96b74eaa..700ba476 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CI609.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI609.html b/models/kt2020_Z1.0_clumpy_M100.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CI609.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CI609.png b/models/kt2020_Z1.0_clumpy_M100.0/CI609.png index 7cdb0ab6..1f1f170d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CI609.png and b/models/kt2020_Z1.0_clumpy_M100.0/CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158.fits b/models/kt2020_Z1.0_clumpy_M100.0/CII158.fits index a64b43ab..10107c1e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158.png index 1ebb1844..1d94a8d6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.png index 3db7a0a6..22eaf152 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.png index 76f0e29a..88ed24d5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.png index 4602bdb9..b9cada98 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.png index 71b4385c..22c2815a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.png index 3f1ebd01..ba3a8eb9 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.png index 94627fb1..e7b6419b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.png index 8686eac3..5f7f360b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO10.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO10.fits index e0517815..92fc430e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO10.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO10.png index a07a72df..4976b3a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO109.fits index 8d5a009d..1e208823 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO109.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109.html b/models/kt2020_Z1.0_clumpy_M100.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO109.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109.png b/models/kt2020_Z1.0_clumpy_M100.0/CO109.png index 1b1d5b6a..8b542cc8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO109.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO109.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.png index 91b30060..6333cb10 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.png index 4657a346..c15a9d05 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.html b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.png b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.png index 1f505052..1229b006 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.fits index 4222dbf2..c55f101c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.png index 3565fa9d..21b4e992 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1110.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.png index 299d8d63..a9c03943 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.png index a01cf53b..c727e7af 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.fits index b2a24347..ba11717f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.png index 91424eae..90697514 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1211.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.png index 7c3f8e70..bd4e86e3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.png index ac88775b..21143410 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.fits index 65199203..48798f16 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.png index 7f153e47..b97b1e69 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1312.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.png index bc895751..d5fb4c12 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.png index ff3e56a7..77011d29 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.fits index 008a7458..84170f6a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.png index f006a7b7..94ad1bbc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1413.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.png index aed89cba..70f493c8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.png index cc9e676d..19ff42f2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO21.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO21.fits index 4ec21897..f2db592b 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO21.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CO21.png index 94c1b9b5..2717ce9e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.png index 7e7b7c71..e0b87386 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO32.fits index 6f798055..1de2568a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO32.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32.html b/models/kt2020_Z1.0_clumpy_M100.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO32.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32.png b/models/kt2020_Z1.0_clumpy_M100.0/CO32.png index 53a02ebd..38d3f149 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO32.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.png index 33a2e1a5..2296c7bf 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.png index 73932dbd..a880bf7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO43.fits index 98315c86..64de49ca 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO43.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43.html b/models/kt2020_Z1.0_clumpy_M100.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO43.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43.png b/models/kt2020_Z1.0_clumpy_M100.0/CO43.png index e1dd4f99..d437fadd 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO43.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.png index 6fce2242..86ff8df3 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.png index 23071d1c..0d131e9d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO54.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO54.fits index 4b2bd1eb..12543b44 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO54.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO54.png index e67feb75..7ad345d1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO65.fits index 6f5d93c5..c5305b1f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO65.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO65.png index 25ff0be8..104e20ea 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.png index 6c63dc93..e74853b8 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.png index 8a48b36d..4acb6dc7 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.png index 148b90aa..29b88d6f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO76.fits index c1ed43d2..259181d5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76.png index 3af760f9..2a68505f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.png index 8689cd49..661a25ae 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.png index 12d68930..77f23b8e 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.png index 7eefea87..4366577d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.png index e5c517f9..5c75ed7c 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.png index 82ce487e..8040b88d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO87.fits index 6a27b7a2..3bc74af4 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO87.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87.html b/models/kt2020_Z1.0_clumpy_M100.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO87.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87.png b/models/kt2020_Z1.0_clumpy_M100.0/CO87.png index f3623e11..a3767e04 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO87.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO87.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.png index dd34a4d3..445e8bef 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.png index 5b349b58..e3c5ca9f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98.fits b/models/kt2020_Z1.0_clumpy_M100.0/CO98.fits index cd9b6985..cc9287a5 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO98.fits and b/models/kt2020_Z1.0_clumpy_M100.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98.html b/models/kt2020_Z1.0_clumpy_M100.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO98.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98.png b/models/kt2020_Z1.0_clumpy_M100.0/CO98.png index 7889d4cc..dd270e31 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO98.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO98.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.html b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.png b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.png index 60283c5f..a95806db 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.html b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.png b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.png index 433aae98..ebdb92a6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.png and b/models/kt2020_Z1.0_clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/FIR.fits b/models/kt2020_Z1.0_clumpy_M100.0/FIR.fits index b2ac4453..f9ad7a28 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/FIR.fits and b/models/kt2020_Z1.0_clumpy_M100.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/FIR.html b/models/kt2020_Z1.0_clumpy_M100.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/FIR.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/FIR.png b/models/kt2020_Z1.0_clumpy_M100.0/FIR.png index 076e0889..6d047c8d 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/FIR.png and b/models/kt2020_Z1.0_clumpy_M100.0/FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.fits b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.fits index 230a60e5..83adf4d1 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.fits and b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.html b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.png b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.png index 23182696..05cc7558 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png index 7412197e..406e4c6a 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145.fits b/models/kt2020_Z1.0_clumpy_M100.0/OI145.fits index ac78f56b..538d40b2 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145.fits and b/models/kt2020_Z1.0_clumpy_M100.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145.html b/models/kt2020_Z1.0_clumpy_M100.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI145.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145.png b/models/kt2020_Z1.0_clumpy_M100.0/OI145.png index a6f3d7ca..5c24e623 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI145.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.html b/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.png b/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.png index 9e0ac30e..fd6cee7f 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.html b/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.png b/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.png index 1b4d9752..b1f3c7ab 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.fits b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.fits index 18e5943b..d7891c47 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.fits and b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.html b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.png b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.png index 274f9f1a..4f3bb0cc 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png index b9093f4c..3211e966 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63.fits b/models/kt2020_Z1.0_clumpy_M100.0/OI63.fits index acf38ec1..eff493df 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63.fits and b/models/kt2020_Z1.0_clumpy_M100.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63.html b/models/kt2020_Z1.0_clumpy_M100.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI63.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63.png b/models/kt2020_Z1.0_clumpy_M100.0/OI63.png index 5f98af81..c0b7cc47 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.html b/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.png b/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.png index 4685f53e..bea313e6 100644 Binary files a/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.png and b/models/kt2020_Z1.0_clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M100.0/index.html b/models/kt2020_Z1.0_clumpy_M100.0/index.html index 20ae284b..cf1054a4 100644 --- a/models/kt2020_Z1.0_clumpy_M100.0/index.html +++ b/models/kt2020_Z1.0_clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI370.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.fits new file mode 100644 index 00000000..5e89cf74 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI370.html b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.html new file mode 100644 index 00000000..6b583693 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI370.png b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.png new file mode 100644 index 00000000..ef24cd39 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CI370.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CI370_CI609.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CI370_CI609.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.html b/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.html new file mode 100644 index 00000000..25504adb --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm/[C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 370 µm/[C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.png b/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.png new file mode 100644 index 00000000..8c09d1a1 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI609.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.fits new file mode 100644 index 00000000..36a98fe8 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI609.html b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.html new file mode 100644 index 00000000..c02944c5 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CI609.png b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.png new file mode 100644 index 00000000..1f1f170d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.fits new file mode 100644 index 00000000..f7b0ba83 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.html new file mode 100644 index 00000000..eac6e844 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.png new file mode 100644 index 00000000..1d94a8d6 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CI609.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CI609.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.html new file mode 100644 index 00000000..e50380ec --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/[C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/[C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.png new file mode 100644 index 00000000..22eaf152 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.html new file mode 100644 index 00000000..438d4afa --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.png new file mode 100644 index 00000000..88ed24d5 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO21.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.html new file mode 100644 index 00000000..079c396c --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.png new file mode 100644 index 00000000..b9cada98 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO32.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO32.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.html new file mode 100644 index 00000000..b0f13434 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.png new file mode 100644 index 00000000..22c2815a Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO43.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO43.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.html new file mode 100644 index 00000000..a74fac52 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=4-3) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.png new file mode 100644 index 00000000..ba3a8eb9 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.html new file mode 100644 index 00000000..4f2b02f0 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=5-4) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.png new file mode 100644 index 00000000..e7b6419b Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CII158_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CII158_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.html new file mode 100644 index 00000000..34ddb3ab --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.png new file mode 100644 index 00000000..5f7f360b Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.fits new file mode 100644 index 00000000..a28db54d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.html new file mode 100644 index 00000000..6f3cfaec --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.png new file mode 100644 index 00000000..4976b3a6 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.fits new file mode 100644 index 00000000..291e4a4f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.html new file mode 100644 index 00000000..cd193d10 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9) Intensity + +
+

+CO(J=10-9) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.png new file mode 100644 index 00000000..8b542cc8 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO109.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO109_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO109_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.html new file mode 100644 index 00000000..71502176 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.png new file mode 100644 index 00000000..6333cb10 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO109_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO109_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.html new file mode 100644 index 00000000..719c5ddf --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.png new file mode 100644 index 00000000..c15a9d05 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO109_CO76.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO109_CO76.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.html new file mode 100644 index 00000000..8820a41b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.png new file mode 100644 index 00000000..1229b006 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.fits new file mode 100644 index 00000000..53caf15a Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.html new file mode 100644 index 00000000..bf05cc5b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.png new file mode 100644 index 00000000..21b4e992 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1110_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1110_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.html new file mode 100644 index 00000000..a46a9556 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.png new file mode 100644 index 00000000..a9c03943 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1110_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1110_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.html new file mode 100644 index 00000000..afecf33e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.png new file mode 100644 index 00000000..c727e7af Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.fits new file mode 100644 index 00000000..d75621bc Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.html new file mode 100644 index 00000000..09b777d0 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11) Intensity + +
+

+CO(J=12-11) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.png new file mode 100644 index 00000000..90697514 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1211_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1211_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.html new file mode 100644 index 00000000..5f3256c8 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.png new file mode 100644 index 00000000..bd4e86e3 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1211_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1211_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.html new file mode 100644 index 00000000..0ee719b3 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.png new file mode 100644 index 00000000..21143410 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.fits new file mode 100644 index 00000000..3340360d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.html new file mode 100644 index 00000000..4b726994 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12) Intensity + +
+

+CO(J=13-12) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.png new file mode 100644 index 00000000..b97b1e69 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1312_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1312_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.html new file mode 100644 index 00000000..7af4dbdf --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.png new file mode 100644 index 00000000..d5fb4c12 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1312_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1312_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.html new file mode 100644 index 00000000..63e2a69c --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.png new file mode 100644 index 00000000..77011d29 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.fits new file mode 100644 index 00000000..5d286996 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.html new file mode 100644 index 00000000..38adb41b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13) Intensity + +
+

+CO(J=14-13) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.png new file mode 100644 index 00000000..cb08db1c Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1413_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1413_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.html new file mode 100644 index 00000000..b99b0e0e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.png new file mode 100644 index 00000000..70f493c8 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO1413_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO1413_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.html new file mode 100644 index 00000000..01f6be6f --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.png new file mode 100644 index 00000000..19ff42f2 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.fits new file mode 100644 index 00000000..1ce6f05c Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.html new file mode 100644 index 00000000..ac801a55 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.png new file mode 100644 index 00000000..2717ce9e Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO21_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO21_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.html new file mode 100644 index 00000000..a91a2d83 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=2-1)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.png new file mode 100644 index 00000000..e0b87386 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.fits new file mode 100644 index 00000000..f03fb3a0 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.html new file mode 100644 index 00000000..3cee5c78 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.png new file mode 100644 index 00000000..38d3f149 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO32.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO32_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO32_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.html new file mode 100644 index 00000000..4644ae2d --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.png new file mode 100644 index 00000000..2296c7bf Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO32_CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO32_CO21.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.html new file mode 100644 index 00000000..b0474ba7 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.png new file mode 100644 index 00000000..a880bf7c Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.fits new file mode 100644 index 00000000..6c084393 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.html new file mode 100644 index 00000000..21d89d5b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.png new file mode 100644 index 00000000..d437fadd Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO43_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO43_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.html new file mode 100644 index 00000000..f582c024 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.png new file mode 100644 index 00000000..86ff8df3 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO43_CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO43_CO21.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.html new file mode 100644 index 00000000..a9ca2bbd --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.png new file mode 100644 index 00000000..0d131e9d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.fits new file mode 100644 index 00000000..b8bed5f1 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.html new file mode 100644 index 00000000..a07c6605 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.png new file mode 100644 index 00000000..7ad345d1 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.fits new file mode 100644 index 00000000..74a17ac2 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.html new file mode 100644 index 00000000..1200eb82 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.png new file mode 100644 index 00000000..104e20ea Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO65_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO65_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.html new file mode 100644 index 00000000..411a5cd3 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.png new file mode 100644 index 00000000..e74853b8 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO65_CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO65_CO21.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.html new file mode 100644 index 00000000..a3bf5a88 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.png new file mode 100644 index 00000000..b06e6607 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO65_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO65_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.html new file mode 100644 index 00000000..4f28f83c --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.png new file mode 100644 index 00000000..29b88d6f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.fits new file mode 100644 index 00000000..72a5c101 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.html new file mode 100644 index 00000000..9ec6ad19 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.png new file mode 100644 index 00000000..2a68505f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO76_CO10.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO76_CO10.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.html new file mode 100644 index 00000000..b95b124e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.png new file mode 100644 index 00000000..661a25ae Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO76_CO21.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO76_CO21.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.html new file mode 100644 index 00000000..5b937735 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.png new file mode 100644 index 00000000..77f23b8e Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO76_CO43.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO76_CO43.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.html new file mode 100644 index 00000000..ee837e7e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.png new file mode 100644 index 00000000..4366577d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO76_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO76_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.html new file mode 100644 index 00000000..8850f65b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.png new file mode 100644 index 00000000..5c75ed7c Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO76_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO76_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.html new file mode 100644 index 00000000..11d57570 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.png new file mode 100644 index 00000000..8040b88d Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.fits new file mode 100644 index 00000000..e6a7a36a Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.html new file mode 100644 index 00000000..57ddc298 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.png new file mode 100644 index 00000000..a3767e04 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO87.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO87_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO87_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.html new file mode 100644 index 00000000..d73c91be --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.png new file mode 100644 index 00000000..445e8bef Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO87_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO87_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.html new file mode 100644 index 00000000..56fd8d37 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.png new file mode 100644 index 00000000..e3c5ca9f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.fits new file mode 100644 index 00000000..227036f8 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.html new file mode 100644 index 00000000..8d2d5e30 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8) Intensity + +
+

+CO(J=9-8) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.png new file mode 100644 index 00000000..dd270e31 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO98.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO98_CO54.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO98_CO54.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.html new file mode 100644 index 00000000..a13db09a --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.png new file mode 100644 index 00000000..a95806db Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/CO98_CO65.fits b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/CO98_CO65.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.html b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.html new file mode 100644 index 00000000..a1963432 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.png b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.png new file mode 100644 index 00000000..ebdb92a6 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/FIR.fits b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.fits new file mode 100644 index 00000000..97a15694 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/FIR.html b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.html new file mode 100644 index 00000000..e95af12b --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+IFIR +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + I<sub>FIR</sub> + +
+

+IFIR emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/FIR.png b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.png new file mode 100644 index 00000000..f6fdc29e Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.fits new file mode 100644 index 00000000..c01d2ea9 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.html new file mode 100644 index 00000000..c7883a50 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm + [C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm + [C II] 158 µm Intensity + +
+

+[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.png new file mode 100644 index 00000000..05cc7558 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/OI145+CII158_FIR.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/OI145+CII158_FIR.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html new file mode 100644 index 00000000..d3397f2e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm + [C II] 158 µm/I<sub>FIR</sub> Intensity Ratio + +
+

+[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png new file mode 100644 index 00000000..c3ae03bc Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.fits new file mode 100644 index 00000000..b98be8c1 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.html new file mode 100644 index 00000000..6b21f4a0 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.png new file mode 100644 index 00000000..5c24e623 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/OI145_CII158.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/OI145_CII158.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.html new file mode 100644 index 00000000..bdc88365 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm/[C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm/[C II] 158 µm Intensity Ratio + +
+

+[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.png new file mode 100644 index 00000000..fd6cee7f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/OI145_OI63.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/OI145_OI63.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.html new file mode 100644 index 00000000..c3d3d721 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm/[O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm/[O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.png new file mode 100644 index 00000000..b1f3c7ab Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.fits new file mode 100644 index 00000000..b79b3a1f Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.html new file mode 100644 index 00000000..d3acd0ee --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm + [C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm + [C II] 158 µm Intensity + +
+

+[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.png new file mode 100644 index 00000000..4f3bb0cc Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/OI63+CII158_FIR.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/OI63+CII158_FIR.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html new file mode 100644 index 00000000..f21bd9b7 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm + [C II] 158 µm/I<sub>FIR</sub> Intensity Ratio + +
+

+[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png new file mode 100644 index 00000000..2b64f39b Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.fits new file mode 100644 index 00000000..2043bed2 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.html new file mode 100644 index 00000000..6978f81e --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.png new file mode 100644 index 00000000..c0b7cc47 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63.png differ diff --git a/models/kt2020_Z1.0_clumpy_M0.0/OI63_CII158.fits b/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.fits similarity index 100% rename from models/kt2020_Z1.0_clumpy_M0.0/OI63_CII158.fits rename to models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.fits diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.html b/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.html new file mode 100644 index 00000000..3e9f2381 --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm/[C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm/[C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.png b/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.png new file mode 100644 index 00000000..bea313e6 Binary files /dev/null and b/models/kt2020_Z1.0_clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_clumpy_M1000.0/index.html b/models/kt2020_Z1.0_clumpy_M1000.0/index.html new file mode 100644 index 00000000..acae908f --- /dev/null +++ b/models/kt2020_Z1.0_clumpy_M1000.0/index.html @@ -0,0 +1,66 @@ + + + + + + + + + +
+
+ +

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, clumpy, maximum clump mass 1000 M⊙, Z=1.0, losangle=0

+

+Below are links to the individual FITS files +and plots in the kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. + +

+ + + + + + + + + + + + + + + + +
[C I] 609 µm Intensity[C I] 370 µm Intensity[O I] 63 µm Intensity[O I] 145 µm Intensity
[C II] 158 µm IntensityCO(J=1-0) IntensityCO(J=2-1) IntensityCO(J=3-2) Intensity
CO(J=4-3) IntensityCO(J=5-4) IntensityCO(J=6-5) IntensityCO(J=7-6) Intensity
CO(J=8-7) IntensityCO(J=9-8) IntensityCO(J=10-9) IntensityCO(J=11-10) Intensity
CO(J=12-11) IntensityCO(J=13-12) IntensityCO(J=14-13) IntensityIFIR
[O I] 63 µm + [C II] 158 µm Intensity[O I] 145 µm + [C II] 158 µm Intensity[O I] 145 µm/[O I] 63 µm Intensity Ratio[O I] 145 µm/[C II] 158 µm Intensity Ratio
[O I] 63 µm/[C II] 158 µm Intensity Ratio[C II] 158 µm/[C I] 609 µm Intensity Ratio[C I] 370 µm/[C I] 609 µm Intensity Ratio[C II] 158 µm/CO(J=1-0) Intensity Ratio
[C II] 158 µm/CO(J=2-1) Intensity Ratio[C II] 158 µm/CO(J=3-2) Intensity Ratio[C II] 158 µm/CO(J=4-3) Intensity Ratio[C II] 158 µm/CO(J=5-4) Intensity Ratio
[C II] 158 µm/CO(J=6-5) Intensity RatioCO(J=2-1)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=2-1) Intensity Ratio
CO(J=4-3)/CO(J=1-0) Intensity RatioCO(J=4-3)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=1-0) Intensity RatioCO(J=6-5)/CO(J=2-1) Intensity Ratio
CO(J=6-5)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=1-0) Intensity RatioCO(J=7-6)/CO(J=2-1) Intensity RatioCO(J=7-6)/CO(J=4-3) Intensity Ratio
CO(J=7-6)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=6-5) Intensity RatioCO(J=8-7)/CO(J=5-4) Intensity RatioCO(J=8-7)/CO(J=6-5) Intensity Ratio
CO(J=9-8)/CO(J=5-4) Intensity RatioCO(J=9-8)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=5-4) Intensity RatioCO(J=10-9)/CO(J=6-5) Intensity Ratio
CO(J=10-9)/CO(J=7-6) Intensity RatioCO(J=11-10)/CO(J=5-4) Intensity RatioCO(J=11-10)/CO(J=6-5) Intensity RatioCO(J=12-11)/CO(J=5-4) Intensity Ratio
CO(J=12-11)/CO(J=6-5) Intensity RatioCO(J=13-12)/CO(J=5-4) Intensity RatioCO(J=13-12)/CO(J=6-5) Intensity RatioCO(J=14-13)/CO(J=5-4) Intensity Ratio
CO(J=14-13)/CO(J=6-5) Intensity Ratio[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio
+

+
+ + + + + diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.fits deleted file mode 100644 index 5bcecc9b..00000000 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.fits and /dev/null differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.html b/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.html deleted file mode 100644 index 6415713a..00000000 --- a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
-
- -

-[C I] 370 µm Intensity -

-

pdrtpy ModelSet: kt2020

-
-
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-
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- - [C I] 370 µm Intensity - -
-

-[C I] 370 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
-
-
-
-
- - - - - - - \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.png b/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.png deleted file mode 100644 index 610ebcf4..00000000 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370.png and /dev/null differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.html deleted file mode 100644 index a7e0b0ac..00000000 --- a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
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- -

-[C I] 370 µm/[C I] 609 µm Intensity Ratio -

-

pdrtpy ModelSet: kt2020

-
-
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-
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- - [C I] 370 µm/[C I] 609 µm Intensity Ratio - -
-

-[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
-
-
-
-
- - - - - - - \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.png deleted file mode 100644 index 08277d63..00000000 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.png and /dev/null differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.fits deleted file mode 100644 index 9bd53007..00000000 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.fits and /dev/null differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.html b/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.html deleted file mode 100644 index abbcd2f2..00000000 --- a/models/kt2020_Z1.0_non-clumpy_M0.0/CI609.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
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- -

-[C I] 609 µm Intensity -

-

pdrtpy ModelSet: kt2020

-
-
-
-
-
-
-
- - [C I] 609 µm Intensity - -
-

-[C I] 609 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
-
-
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-[C II] 158 µm Intensity -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/[C I] 609 µm Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=1-0) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=3-2) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=4-3) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[C II] 158 µm/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=1-0) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=1-0) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=10-9) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=10-9) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=10-9)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=10-9)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=10-9)/CO(J=7-6) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=11-10) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=11-10)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=11-10)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=12-11) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=12-11) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=12-11)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-

-CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=12-11)/CO(J=6-5) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

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- - CO(J=12-11)/CO(J=6-5) Intensity Ratio - -
-

-CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=13-12) Intensity -

-

pdrtpy ModelSet: kt2020

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-

-CO(J=13-12) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=13-12)/CO(J=5-4) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

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-

-CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=13-12)/CO(J=6-5) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

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-

-CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=14-13) Intensity -

-

pdrtpy ModelSet: kt2020

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-

-CO(J=14-13) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=14-13)/CO(J=5-4) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

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-CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=14-13)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-

-CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=2-1) Intensity -

-

pdrtpy ModelSet: kt2020

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-CO(J=2-1) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=2-1)/CO(J=1-0) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

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-CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=3-2) Intensity -

-

pdrtpy ModelSet: kt2020

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-

-CO(J=3-2) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=3-2)/CO(J=1-0) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

-
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-

-CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=3-2)/CO(J=2-1) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

-
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-

-CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=4-3) Intensity -

-

pdrtpy ModelSet: kt2020

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-CO(J=4-3) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

-
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-CO(J=4-3)/CO(J=1-0) Intensity Ratio -

-

pdrtpy ModelSet: kt2020

-
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- - CO(J=4-3)/CO(J=1-0) Intensity Ratio - -
-

-CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=4-3)/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=5-4) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=5-4) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=6-5) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=6-5)/CO(J=1-0) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=6-5)/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=6-5)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=1-0) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=2-1) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=4-3) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=5-4) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=7-6)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=8-7) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=8-7)/CO(J=6-5) Intensity Ratio -

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pdrtpy ModelSet: kt2020

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-CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-CO(J=9-8) Intensity -

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pdrtpy ModelSet: kt2020

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-CO(J=9-8) Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

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-[O I] 63 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-[O I] 63 µm/[C II] 158 µm Intensity Ratio -

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-[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. -

-The FITS file is available for download. -

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-KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0

-

-Below are links to the individual FITS files -and plots in the kt2020 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. - - - - - - - - - - - - - - - - - - -
[C I] 609 µm Intensity[C I] 370 µm Intensity[O I] 63 µm Intensity[O I] 145 µm Intensity
[C II] 158 µm IntensityCO(J=1-0) IntensityCO(J=2-1) IntensityCO(J=3-2) Intensity
CO(J=4-3) IntensityCO(J=5-4) IntensityCO(J=6-5) IntensityCO(J=7-6) Intensity
CO(J=8-7) IntensityCO(J=9-8) IntensityCO(J=10-9) IntensityCO(J=11-10) Intensity
CO(J=12-11) IntensityCO(J=13-12) IntensityCO(J=14-13) IntensityIFIR
[O I] 63 µm + [C II] 158 µm Intensity[O I] 145 µm + [C II] 158 µm IntensitySurface Temperature[O I] 145 µm/[O I] 63 µm Intensity Ratio
[O I] 145 µm/[C II] 158 µm Intensity Ratio[O I] 63 µm/[C II] 158 µm Intensity Ratio[C II] 158 µm/[C I] 609 µm Intensity Ratio[C I] 370 µm/[C I] 609 µm Intensity Ratio
[C II] 158 µm/CO(J=1-0) Intensity Ratio[C II] 158 µm/CO(J=2-1) Intensity Ratio[C II] 158 µm/CO(J=3-2) Intensity Ratio[C II] 158 µm/CO(J=4-3) Intensity Ratio
[C II] 158 µm/CO(J=5-4) Intensity Ratio[C II] 158 µm/CO(J=6-5) Intensity RatioCO(J=2-1)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=1-0) Intensity Ratio
CO(J=3-2)/CO(J=2-1) Intensity RatioCO(J=4-3)/CO(J=1-0) Intensity RatioCO(J=4-3)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=1-0) Intensity Ratio
CO(J=6-5)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=1-0) Intensity RatioCO(J=7-6)/CO(J=2-1) Intensity Ratio
CO(J=7-6)/CO(J=4-3) Intensity RatioCO(J=7-6)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=6-5) Intensity RatioCO(J=8-7)/CO(J=5-4) Intensity Ratio
CO(J=8-7)/CO(J=6-5) Intensity RatioCO(J=9-8)/CO(J=5-4) Intensity RatioCO(J=9-8)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=5-4) Intensity Ratio
CO(J=10-9)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=7-6) Intensity RatioCO(J=11-10)/CO(J=5-4) Intensity RatioCO(J=11-10)/CO(J=6-5) Intensity Ratio
CO(J=12-11)/CO(J=5-4) Intensity RatioCO(J=12-11)/CO(J=6-5) Intensity RatioCO(J=13-12)/CO(J=5-4) Intensity RatioCO(J=13-12)/CO(J=6-5) Intensity Ratio
CO(J=14-13)/CO(J=5-4) Intensity RatioCO(J=14-13)/CO(J=6-5) Intensity Ratio[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio
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- - - - diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.fits index 119258f8..acde9a46 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.png index cbec6b93..a7351b37 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.png index daa2ec57..b54cb1ec 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.fits index d1a1435e..b1bcdec0 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.png index ee6f262c..bbf81d18 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.fits index ac50de2e..5695b72f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.png index 32349bbb..8604b0d3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.png index 7b32411c..ac988f1c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.png index 8c2ec725..64dfe10f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.png index 28947e5e..e0137031 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.png index 4a7cc459..67b05de7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.png index a74cfb67..52f09b90 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.png index e3a7ba2f..27c64bf3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.png index 4623daf9..49d13b2e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.fits index 68c3d76d..b412cdc9 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.png index d017f51e..93c812a8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.fits index ffa47be0..7ae7f491 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.png index eb73453f..b61ce57f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.png index 588a332c..91df4514 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.png index 06c8c312..8bdd07a4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.png index 4cafcc63..c9ecd32a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.fits index f82f0962..175641df 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.png index 0970e92e..9d6c75c8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.png index f57ca386..b5b8492c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.png index 72f29aec..d72fea4a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.fits index cfaa8479..29186dfa 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.png index a74b0c7c..e8fc4f99 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.png index cc545f47..86f75fa6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.png index ab320408..f12cf959 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.fits index ec4a8c77..9d0ab153 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.png index 3cccf267..6456f92c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.png index e6185083..c7ed5250 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.png index df4aefae..cfd1cbfb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.fits index c33a35fa..1a65fc1b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.png index 3875b279..d5ebd9a5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.png index 90d13035..3d74d600 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.png index 9284e4a7..6c8672b7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.fits index 85bd6fc0..5145cc4d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.png index 3547eb78..bab5458a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.png index 0c98824b..537c51a0 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.fits index eeffc263..e7115bce 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.png index 3bc3f607..b1a94887 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.png index 1c1faf45..7c59b3fb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.png index f85ddd89..496fa627 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.fits index 7423b6cc..9d476a07 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.png index 9d921ffe..63faffbb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.png index ef88837a..1782bbbe 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.png index 1be55ec5..a91a0aca 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.fits index 2f2ddec1..e450c0ba 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.png index 8f6f00c7..5b7b3bb4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.fits index b76304c9..344ca040 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.png index 8b9ae21e..67187a35 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.png index 1a32eef7..1f10fa2c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.png index ec18f18f..94b557d9 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.png index 65865b2c..d6bf77b4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.fits index a31a6a1f..8d79c290 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.png index 0ab32f5c..5a2f3fea 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.png index 1c33d2f5..5b5d9969 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.png index cd69846a..ffec1c00 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.png index d9c445b0..a1a88384 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.png index b666f480..6b9f5883 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.png index badde18b..9b1be36e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.fits index 9e6b6113..9c16cd24 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.png index 05838f61..f3c6f21f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.png index 76f942a3..f4d809f6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.png index 7239378e..041ea0c2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.fits index 5e32ec01..2aa1341c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.png index 8da1dad0..9368d1ba 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.png index 29225cfb..a50080fe 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.html b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.png b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.png index a219f52b..c084268d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.fits index ee41a3cf..6cbb0b71 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.html b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.png b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.png index 3b60aeab..29ed0f6e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.fits index 3d3c92f2..7b138420 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.png index 882fa1aa..2e4841a3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png index e4f69999..f7dadd6f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.fits index e2ad9ff4..925ff8b5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.png index cf55e79b..7502dfe6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.png index e9914cf2..20e6acc9 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.png index 543399fb..9233c1bb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.fits index 65ed119c..95a36a48 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.png index b561f442..7deb601a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png index 22179674..23975934 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.fits b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.fits index 83b9ace2..a782ca3e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.fits and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.png index abe8cb6f..bea5cc07 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.html b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.png b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.png index d50bdd1a..eda3df4b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.html b/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.html index 3b3c6950..fd0aabfb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.png b/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.png index f18c675c..b4e173f5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.png and b/models/kt2020_Z1.0_non-clumpy_M0.1/Ts.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.1/index.html b/models/kt2020_Z1.0_non-clumpy_M0.1/index.html index 45173983..6f4f93aa 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.1/index.html +++ b/models/kt2020_Z1.0_non-clumpy_M0.1/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 0.1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.fits index 660472a8..36331b40 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.png index a47ab1ad..d88ab20e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.png index 796d2ebb..893ee7c5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.fits index 5b56353c..7f0b8cc4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.png index 73f7fd57..fbbf96b8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.fits index 2d63b5ce..85f8c7ab 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.png index d7baf244..10057fce 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.png index ca5a3683..5eb14014 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.png index caea9cc7..4094c9ab 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.png index de7aad2e..8a920bbf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.png index 339ecf2d..a937ddf3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.png index 556d51df..790416b7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.png index 98b3979b..1b2f8865 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.png index 275fde83..7e89525c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.fits index ee291f09..193d5e4b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.png index b374bac5..f3fac681 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.fits index d02abf2b..000fbd48 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.png index b0c9bedd..ffdba6b2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.png index 3d2453a3..63ca8e76 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.png index 5bd3fba7..39252280 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.png index ba15221b..ea541325 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.fits index e6dd34e8..dc595696 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.png index 38e2acfa..7cc85c95 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.png index 04a0bbe7..050331f1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.png index b2637428..8bebdfe7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.fits index 9ab37c04..2a32cf28 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.png index d9cdeabe..e7c4d672 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.png index 88498a13..c9ded859 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.png index 2c5c8461..7788fd63 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.fits index 69af0581..8adf3937 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.png index 640a03e3..8cbd8be2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.png index 79a9f863..350f80bf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.png index ad3bfcd0..96140bb8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.fits index de698ae1..f17d90ef 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.png index 544b1b94..4853a630 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.png index 4ccdfbfd..0fb60133 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.png index fb687350..0dd46d85 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.fits index a7297548..0a21cb30 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.png index ecf81695..8a5d5b1b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.png index 54bf37f6..0bd81914 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.fits index 57a9cda2..127fb521 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.png index 44f55051..ab84e55b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.png index fe196d8d..4bc2198a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.png index f69c0cc2..f1864c9b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.fits index 7a646138..49700d25 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.png index b8bec9fa..8e27a4cd 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.png index 2252696c..077a5169 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.png index 87a2e304..d5f6dc6d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.fits index 8d6e9497..4a80d004 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.png index 795d9702..fad9bf7c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.fits index f8fe087f..154ddf20 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.png index 40d55b5e..92b5b2e9 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.png index f9ef4f5c..777c1a2b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.png index 0162c459..0d11bddf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.png index 27a44e98..0ec65420 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.fits index a9ff5b10..830480ce 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.png index 3172bec7..6ff54f75 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.png index 55bf516d..be939ecc 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.png index 93f087da..7db394a6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.png index 46cccd81..7b816f13 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.png index 5c407fcf..34c76848 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.png index dee25b49..61e810ee 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.fits index 42586274..b359ca36 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.png index f5e84d05..bd303828 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.png index b94a376f..a5264016 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.png index f8ae43e0..78a25651 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.fits index 0248c07a..9217a28d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.png index 46253753..74e67577 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.png index a6e71abe..aa1fb66c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.png index a5b0fcc9..83b5fb43 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.fits index ab8bd3c7..fd0dd924 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.html b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.png b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.png index 0af76e75..a101f086 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.fits index 86f3fceb..29434bfd 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.png index c8429295..2c28e2ca 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png index 4fca0d28..9a33b236 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.fits index 1318772e..b133e9c3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.png index 12f931ff..fdddebf9 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.png index 8f8de2ee..aa6546ca 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.png index dc194075..de3e5a3e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.fits index a3125ed0..cfd8f134 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.png index ce8cf665..43b08f20 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png index e2e3b9f4..f1cb6fc5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.fits b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.fits index 450a5d06..d0c7c19a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.fits and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.png index 4550d58c..45e6c1bf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.html b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.png b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.png index adb19491..4733e903 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.html b/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.html index 3b3c6950..fd0aabfb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.png b/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.png index 08b428b2..6c2d23b7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.png and b/models/kt2020_Z1.0_non-clumpy_M1.0/Ts.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1.0/index.html b/models/kt2020_Z1.0_non-clumpy_M1.0/index.html index 5615a613..1ff3a99e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M1.0/index.html +++ b/models/kt2020_Z1.0_non-clumpy_M1.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.fits index 758cba33..8bd2cb01 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.png index b083b076..7ef93616 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.png index 008c5d3d..3a9997ab 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.fits index 4a257002..64a0ab3a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.png index 335a170a..b9067ffe 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.fits index 17cf1e60..6e0d1e96 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.png index fb4125fc..83b9788b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.png index 89288ebc..da236098 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.png index f96f0061..639a96d2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.png index daf54b2b..18c24f11 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.png index c858f46c..75546a28 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.png index b0609795..578363a6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.png index c63fae7b..d5873789 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.png index 6a938c3b..9ea827f1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.fits index 6e01b8cd..7e0f7421 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.png index c526cd63..11ad1ac1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.fits index e1f2e9ff..92584e37 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.png index d24a3f6b..eba17b70 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.png index 926cb542..23d6171b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.png index 4e7c6613..a177b351 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.png index f57b9b16..6243b9e2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.fits index c46a1d7f..f3d0c486 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.png index c1bbd6db..3dc10a4a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.png index 0148e383..e8601e13 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.png index 9594629e..9eb72cc3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.fits index 52292f62..cada66f8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.png index 61694d22..9b41ba0e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.png index c9a848f3..867ea002 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.png index db5765f1..944b48da 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.fits index deaf41ed..cf1d27ce 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.png index 47accbde..6b498c2e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.png index fabc4c52..b128a3ce 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.png index 76630666..3b77554a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.fits index 50a93978..3ba1210b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.png index fc53a859..5a0c6c58 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.png index 1f88163a..276cd7ab 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.png index 23df3bf3..6b92cbeb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.fits index 55d5f4c4..a7dcf3a6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.png index 9bb7fe23..85270525 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.png index d26c3937..b130b7a4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.fits index e34ea2d5..1ed2e133 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.png index 8de96695..46fcdb70 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.png index 1f67751a..8ff10b7b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.png index 269bea6c..5fbebbbe 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.fits index 6014bbb1..d9ce5805 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.png index 077f3557..cb642a0d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.png index e2c06e07..456a0333 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.png index 5a9ec9f8..13498f46 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.fits index d963ff30..e600cb50 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.png index ad4e620b..8f7626d6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.fits index 73f32ee4..32a0d56c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.png index c8f3aea8..44c38764 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.png index 6c26cac6..2d3bb876 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.png index 5bcc62f5..83bf3732 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.png index 2cb4de38..ab6198b6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.fits index e49f22a2..d72785a6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.png index f604f76d..dacd6509 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.png index 528125fb..66683a94 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.png index d0f7d363..aaa15ccd 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.png index 36aac64f..9b1b7045 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.png index eef248a8..de288c0b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.png index 357207bd..b5e171d4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.fits index 43d2c2df..2b12ad9d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.png index a87901de..d7c5725a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.png index 72145b7d..e95c2a6f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.png index b8386bfe..c9c211cd 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.fits index 507d2151..bc20dfb3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.png index 396e73c5..e6514cb5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.png index cce7ae2b..0f997089 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.html b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.png b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.png index ea6f41a5..650a3eaa 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.fits index 007cf06e..3f1f353a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.html b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.png b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.png index c6c69b44..2dedb80a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.fits index 5a49cbda..d0f2201d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.png index 6ff44114..047f4c65 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png index 30e79b06..46227e5a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.fits index 828e43c5..ca0884b3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.png index 2e066cef..9a098083 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.png index 5e8b4c92..901d5f3e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.png index f552ba3d..ba5b4ee4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.fits index 06d197c2..b13eaf25 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.png index 465d71a7..62e5511e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png index b0da286b..ba11e767 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.fits b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.fits index 0e9bb8eb..8e4fc8b4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.fits and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.png index dac904a3..e5b61802 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.html b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.png b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.png index 96fd599d..92e0d653 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.html b/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.html index 3b3c6950..fd0aabfb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.png b/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.png index c3d463b5..ed15cc49 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.png and b/models/kt2020_Z1.0_non-clumpy_M10.0/Ts.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M10.0/index.html b/models/kt2020_Z1.0_non-clumpy_M10.0/index.html index f841800d..a39b8f91 100644 --- a/models/kt2020_Z1.0_non-clumpy_M10.0/index.html +++ b/models/kt2020_Z1.0_non-clumpy_M10.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 10 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.fits index 8f47208b..e85afdd3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.html index 6415713a..6b583693 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.html @@ -47,6 +47,7 @@

[C I] 370 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.png index 7a0125fe..19444815 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.html index a7e0b0ac..25504adb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.html @@ -47,6 +47,7 @@

[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.png index 39115dfa..557a24d4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.fits index 439d00d5..1675a9c7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.html index abbcd2f2..c02944c5 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.html @@ -47,6 +47,7 @@

[C I] 609 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.png index c7bc6196..0e27f1cf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.fits index 1a1ae781..d7e9e5f7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.html index b4e12ab1..eac6e844 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.html @@ -47,6 +47,7 @@

[C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.png index 5020a0bf..e86cd688 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.html index 1223976c..e50380ec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.html @@ -47,6 +47,7 @@

[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.png index 8b6b54cd..3fb401a4 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.html index 41525fe5..438d4afa 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.png index 15d2b9d9..3a5db16b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.html index ef4d9798..079c396c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.png index a16f4567..fed389f6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.html index 0e014f33..b0f13434 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.png index 3ff48f2b..5e50c44d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.html index 33ece0e6..a74fac52 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.png index 3fc81515..54cf7210 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.html index 2c5cdeff..4f2b02f0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.png index ec1ccace..1ca558a6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.html index 252217a1..34ddb3ab 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.html @@ -47,6 +47,7 @@

[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.png index cb65f0a5..53b0dc87 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.fits index b5881edf..208ee5e2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.html index 77094a4f..6f3cfaec 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.html @@ -47,6 +47,7 @@

CO(J=1-0) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.png index 689459e5..ddd9eb34 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.fits index 4818caad..c965419e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.html index 84b98253..cd193d10 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.html @@ -47,6 +47,7 @@

CO(J=10-9) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.png index fc28514d..ad85d3bb 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.html index 62481db2..71502176 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.png index b6f9ae69..69019f96 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.html index 749541b1..719c5ddf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.png index 4299dabf..d7c350fc 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.html index f32374e5..8820a41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.html @@ -47,6 +47,7 @@

CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.png index 20464a3a..3feeaa72 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.fits index 65bba17b..5f162794 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.html index 211bc8cb..bf05cc5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.html @@ -47,6 +47,7 @@

CO(J=11-10) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.png index 4c8a6eab..56be9aa1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.html index 4bfe9aed..a46a9556 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.png index 5fc3f275..bfff4f6a 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.html index 4e416e5a..afecf33e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.html @@ -47,6 +47,7 @@

CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.png index 96eda826..4e1428f2 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.fits index bc293329..20a08618 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.html index 3d461d1e..09b777d0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.html @@ -47,6 +47,7 @@

CO(J=12-11) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.png index 3211e980..04177c1d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.html index 6ec21a53..5f3256c8 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.png index 82494084..e6d0f00c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.html index f0a8be13..0ee719b3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.html @@ -47,6 +47,7 @@

CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.png index d4052a20..2bda15b0 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.fits index de887528..79645a93 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.html index 9a540a58..4b726994 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.html @@ -47,6 +47,7 @@

CO(J=13-12) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.png index 1806a971..c496329c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.html index 7c046ce6..7af4dbdf 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.png index e5b44bc8..a3c33576 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.html index 0b903461..63e2a69c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.html @@ -47,6 +47,7 @@

CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.png index 1024d678..426f2d24 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.fits index fbf27ab9..3288c0fa 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.html index 460086e6..38adb41b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.html @@ -47,6 +47,7 @@

CO(J=14-13) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.png index 28aec730..932a2037 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.html index dd3f829a..b99b0e0e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.png index 0244b50a..6e275e59 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.html index c425e485..01f6be6f 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.html @@ -47,6 +47,7 @@

CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.png index ae46522c..f03d14f1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.fits index 42f5ca8a..b1a91053 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.html index 73b16d5f..ac801a55 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.html @@ -47,6 +47,7 @@

CO(J=2-1) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.png index 9040eac1..77a71988 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.html index 2225b95f..a91a2d83 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.html @@ -47,6 +47,7 @@

CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.png index e4ee0407..309bc3a8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.fits index 9f87b7bb..e74d7683 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.html index 06a74ee1..3cee5c78 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.html @@ -47,6 +47,7 @@

CO(J=3-2) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.png index 03121186..ce7d3f37 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.html index 82773718..4644ae2d 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.png index 26a582f3..2394029c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.html index 40872e23..b0474ba7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.html @@ -47,6 +47,7 @@

CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.png index 2519b784..cba3edb1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.fits index 45172e4a..502d52c5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.html index eccdb3a3..21d89d5b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.html @@ -47,6 +47,7 @@

CO(J=4-3) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.png index 62cff788..b4202479 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.html index 4a4fb97a..f582c024 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.png index 56e19180..d93d4d85 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.html index dd35e99a..a9ca2bbd 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.html @@ -47,6 +47,7 @@

CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.png index fe2f045e..0a5df25b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.fits index fe59c392..5dddc46e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.html index 47b2c113..a07c6605 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.html @@ -47,6 +47,7 @@

CO(J=5-4) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.png index 278f34aa..4d7b93e1 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.fits index b806ecb2..fec3c814 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.html index 0d0e5e56..1200eb82 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.html @@ -47,6 +47,7 @@

CO(J=6-5) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.png index f4b7e532..82c32561 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.html index e71fee1d..411a5cd3 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.png index 0bb189cc..68ae6fe3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.html index 13fd7bc5..a3bf5a88 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.png index bff22872..0d2f3377 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.html index b2bd2fe5..4f28f83c 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.html @@ -47,6 +47,7 @@

CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.png index ecb743a8..c6ba42e8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.fits index e5a5f6f9..e5bd8c21 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.html index 2be56a7c..9ec6ad19 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.html @@ -47,6 +47,7 @@

CO(J=7-6) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.png index 0c8712f2..8f8eb0b8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.html index bd21d44d..b95b124e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.png index 955ec985..6fcd5d6f 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.html index 8cdc97d0..5b937735 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.png index 32b39c6d..b93318ff 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.html index 9b92fa49..ee837e7e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.png index 34c5e808..44e6a20b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.html index 8ce73f28..8850f65b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.png index 20c31413..c2edc6cf 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.html index 7a3511f4..11d57570 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.html @@ -47,6 +47,7 @@

CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.png index 0209f061..51de4576 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.fits index af7b499f..80a390c8 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.html index 77f74ee0..57ddc298 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.html @@ -47,6 +47,7 @@

CO(J=8-7) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.png index a888f24d..9636dcf6 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.html index a35e0717..d73c91be 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.png index 8cb8cd27..6f60541c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.html index 44446c80..56fd8d37 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.html @@ -47,6 +47,7 @@

CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.png index c1d21d48..ee5bb719 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.fits index c8514495..d4df470c 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.html index 040d5e41..8d2d5e30 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.html @@ -47,6 +47,7 @@

CO(J=9-8) Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.png index 6e515dbe..b307a4ca 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.html index 21dacf62..a13db09a 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.png index 4c2b703a..fd77de24 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.html b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.html index e7c42945..a1963432 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.html @@ -47,6 +47,7 @@

CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.png b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.png index 97bb80b7..a5485333 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.fits index e4ce3f48..83e485a5 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.html b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.html index 3982b817..e95af12b 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.html @@ -47,6 +47,7 @@

IFIR emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.png b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.png index 076e0889..6d047c8d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.fits index f76ada71..d1e1bef3 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.html index bbaea6b3..c7883a50 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.png index f793ee8a..4a7e1a09 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html index 7fa527c0..d3397f2e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png index 6b64cda4..a0add4ea 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.fits index ceefc17f..99548453 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.html index 87792c14..6b21f4a0 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.html @@ -47,6 +47,7 @@

[O I] 145 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.png index 2ea39f61..6f283f23 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.html index 465a1a29..bdc88365 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.html @@ -47,6 +47,7 @@

[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.png index 221aa0bf..f2e1dd2e 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.html index 04ecb0a0..c3d3d721 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.html @@ -47,6 +47,7 @@

[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.png index 238761b2..183211e7 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.fits index 933504df..72ef7459 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.html index f8b9bb37..d3acd0ee 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.png index ed7bbb29..7a051b6d 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html index f7d17a00..f21bd9b7 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.html @@ -47,6 +47,7 @@

[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png index da69e626..35998d05 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.fits b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.fits index 557dfed8..f6430100 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.fits and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.html index 14474cc7..6978f81e 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.html @@ -47,6 +47,7 @@

[O I] 63 µm Intensity emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.png index 10c98032..ef2de35b 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.html b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.html index 19fbfaf4..3e9f2381 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.html @@ -47,6 +47,7 @@

[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.png b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.png index 3177827f..a7712799 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.html b/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.html index 3b3c6950..fd0aabfb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.png b/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.png index 7841bcad..b3fcf404 100644 Binary files a/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.png and b/models/kt2020_Z1.0_non-clumpy_M100.0/Ts.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M100.0/index.html b/models/kt2020_Z1.0_non-clumpy_M100.0/index.html index 1b399b69..b8726aea 100644 --- a/models/kt2020_Z1.0_non-clumpy_M100.0/index.html +++ b/models/kt2020_Z1.0_non-clumpy_M100.0/index.html @@ -33,10 +33,10 @@

-KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 100 M⊙, Z=1.0, losangle=0

Below are links to the individual FITS files -and plots in the kt2020 kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files.

diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.fits new file mode 100644 index 00000000..819b3570 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.html new file mode 100644 index 00000000..6b583693 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.png new file mode 100644 index 00000000..4219bf83 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CI370_CI609.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.html new file mode 100644 index 00000000..25504adb --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm/[C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 370 µm/[C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.png new file mode 100644 index 00000000..2199f3b3 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI370_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.fits new file mode 100644 index 00000000..7c494e43 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.html new file mode 100644 index 00000000..c02944c5 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.png new file mode 100644 index 00000000..9280b8d0 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.fits new file mode 100644 index 00000000..9a42b57d Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.html new file mode 100644 index 00000000..eac6e844 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.png new file mode 100644 index 00000000..01cec11f Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CI609.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CI609.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.html new file mode 100644 index 00000000..e50380ec --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/[C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/[C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm/[C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.png new file mode 100644 index 00000000..acab71b3 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CI609.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.html new file mode 100644 index 00000000..438d4afa --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.png new file mode 100644 index 00000000..aee6fe22 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO21.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.html new file mode 100644 index 00000000..079c396c --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.png new file mode 100644 index 00000000..bd347aa3 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO32.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO32.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.html new file mode 100644 index 00000000..b0f13434 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.png new file mode 100644 index 00000000..d6607e91 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO43.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO43.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.html new file mode 100644 index 00000000..a74fac52 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=4-3) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.png new file mode 100644 index 00000000..e39aa932 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.html new file mode 100644 index 00000000..4f2b02f0 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=5-4) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.png new file mode 100644 index 00000000..7115b433 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CII158_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.html new file mode 100644 index 00000000..34ddb3ab --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [C II] 158 µm/CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.png new file mode 100644 index 00000000..10961163 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CII158_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.fits new file mode 100644 index 00000000..e7893b13 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.html new file mode 100644 index 00000000..6f3cfaec --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.png new file mode 100644 index 00000000..b4d28a59 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.fits new file mode 100644 index 00000000..11ae2ce9 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.html new file mode 100644 index 00000000..cd193d10 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9) Intensity + +
+

+CO(J=10-9) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.png new file mode 100644 index 00000000..a0774c69 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.html new file mode 100644 index 00000000..71502176 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.png new file mode 100644 index 00000000..bc63165a Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.html new file mode 100644 index 00000000..719c5ddf --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.png new file mode 100644 index 00000000..46af946e Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO76.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO109_CO76.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.html new file mode 100644 index 00000000..8820a41b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9)/CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=10-9)/CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9)/CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.png new file mode 100644 index 00000000..e4a54b09 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO109_CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.fits new file mode 100644 index 00000000..f3468e1b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.html new file mode 100644 index 00000000..bf05cc5b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.png new file mode 100644 index 00000000..6ace37a3 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1110_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1110_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html new file mode 100644 index 00000000..a46a9556 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png new file mode 100644 index 00000000..1580f3f7 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1110_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1110_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html new file mode 100644 index 00000000..afecf33e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=11-10)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png new file mode 100644 index 00000000..df75c617 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1110_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.fits new file mode 100644 index 00000000..67728a95 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.html new file mode 100644 index 00000000..09b777d0 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11) Intensity + +
+

+CO(J=12-11) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.png new file mode 100644 index 00000000..845a1fe6 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1211_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1211_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html new file mode 100644 index 00000000..5f3256c8 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png new file mode 100644 index 00000000..f9c7f138 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1211_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1211_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html new file mode 100644 index 00000000..0ee719b3 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=12-11)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png new file mode 100644 index 00000000..b9125c05 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1211_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.fits new file mode 100644 index 00000000..aaf8000d Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.html new file mode 100644 index 00000000..4b726994 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12) Intensity + +
+

+CO(J=13-12) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.png new file mode 100644 index 00000000..26f8953c Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1312_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1312_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html new file mode 100644 index 00000000..7af4dbdf --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png new file mode 100644 index 00000000..0fc8c286 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1312_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1312_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html new file mode 100644 index 00000000..63e2a69c --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=13-12)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png new file mode 100644 index 00000000..60f4364b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1312_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.fits new file mode 100644 index 00000000..3ad61692 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.html new file mode 100644 index 00000000..38adb41b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13) Intensity + +
+

+CO(J=14-13) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.png new file mode 100644 index 00000000..628f05bf Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1413_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1413_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html new file mode 100644 index 00000000..b99b0e0e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png new file mode 100644 index 00000000..d9646774 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO1413_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO1413_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html new file mode 100644 index 00000000..01f6be6f --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=14-13)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png new file mode 100644 index 00000000..4edb22d2 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO1413_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.fits new file mode 100644 index 00000000..c809a5c9 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.html new file mode 100644 index 00000000..ac801a55 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.png new file mode 100644 index 00000000..c8c8dd3f Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO21_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO21_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.html new file mode 100644 index 00000000..a91a2d83 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=2-1)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.png new file mode 100644 index 00000000..4785341a Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO21_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.fits new file mode 100644 index 00000000..7e2bc9ce Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.html new file mode 100644 index 00000000..3cee5c78 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.png new file mode 100644 index 00000000..de25878b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO32_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO32_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.html new file mode 100644 index 00000000..4644ae2d --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.png new file mode 100644 index 00000000..fe02dc4f Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO32_CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO32_CO21.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.html new file mode 100644 index 00000000..b0474ba7 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=3-2)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.png new file mode 100644 index 00000000..74d9dc01 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO32_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.fits new file mode 100644 index 00000000..6edf6c9c Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.html new file mode 100644 index 00000000..21d89d5b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.png new file mode 100644 index 00000000..6eba8e96 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO43_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO43_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.html new file mode 100644 index 00000000..f582c024 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=4-3)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.png new file mode 100644 index 00000000..74944f0c Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO43_CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO43_CO21.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.html new file mode 100644 index 00000000..a9ca2bbd --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=4-3)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.png new file mode 100644 index 00000000..34474727 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO43_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.fits new file mode 100644 index 00000000..a16352ba Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.html new file mode 100644 index 00000000..a07c6605 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.png new file mode 100644 index 00000000..7c1d55fb Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.fits new file mode 100644 index 00000000..09fe5db0 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.html new file mode 100644 index 00000000..1200eb82 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.png new file mode 100644 index 00000000..28d16521 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.html new file mode 100644 index 00000000..411a5cd3 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.png new file mode 100644 index 00000000..933e14d9 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO21.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.html new file mode 100644 index 00000000..a3bf5a88 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.png new file mode 100644 index 00000000..e0aae6f1 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO65_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.html new file mode 100644 index 00000000..4f28f83c --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=6-5)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=6-5)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.png new file mode 100644 index 00000000..d21018f2 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO65_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.fits new file mode 100644 index 00000000..f103f560 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.html new file mode 100644 index 00000000..9ec6ad19 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.png new file mode 100644 index 00000000..efcae995 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO10.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO10.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.html new file mode 100644 index 00000000..b95b124e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.png new file mode 100644 index 00000000..356837e2 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO10.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO21.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO21.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.html new file mode 100644 index 00000000..5b937735 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.png new file mode 100644 index 00000000..69b9c496 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO21.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO43.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO43.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.html new file mode 100644 index 00000000..ee837e7e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.png new file mode 100644 index 00000000..9b623b80 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO43.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.html new file mode 100644 index 00000000..8850f65b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.png new file mode 100644 index 00000000..c052b166 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO76_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.html new file mode 100644 index 00000000..11d57570 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=7-6)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.png new file mode 100644 index 00000000..1bc30e02 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO76_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.fits new file mode 100644 index 00000000..6ddfa22d Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.html new file mode 100644 index 00000000..57ddc298 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.png new file mode 100644 index 00000000..e3a92759 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO87_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO87_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.html new file mode 100644 index 00000000..d73c91be --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.png new file mode 100644 index 00000000..285ea365 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO87_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO87_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.html new file mode 100644 index 00000000..56fd8d37 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=8-7)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.png new file mode 100644 index 00000000..bafbfc6b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO87_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.fits new file mode 100644 index 00000000..24c38e74 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.html new file mode 100644 index 00000000..8d2d5e30 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8) Intensity + +
+

+CO(J=9-8) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.png new file mode 100644 index 00000000..f6a92232 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO98_CO54.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO98_CO54.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.html new file mode 100644 index 00000000..a13db09a --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8)/CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8)/CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8)/CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.png new file mode 100644 index 00000000..4e41c789 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO54.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/CO98_CO65.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/CO98_CO65.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.html new file mode 100644 index 00000000..a1963432 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8)/CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + CO(J=9-8)/CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8)/CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.png new file mode 100644 index 00000000..89a7d9e6 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/CO98_CO65.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.fits new file mode 100644 index 00000000..69eb7619 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.html new file mode 100644 index 00000000..e95af12b --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+IFIR +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + I<sub>FIR</sub> + +
+

+IFIR emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.png new file mode 100644 index 00000000..f6fdc29e Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits new file mode 100644 index 00000000..7f122961 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.html new file mode 100644 index 00000000..c7883a50 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm + [C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm + [C II] 158 µm Intensity + +
+

+[O I] 145 µm + [C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.png new file mode 100644 index 00000000..c8edbc57 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/OI145+CII158_FIR.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/OI145+CII158_FIR.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html new file mode 100644 index 00000000..d3397f2e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm + [C II] 158 µm/I<sub>FIR</sub> Intensity Ratio + +
+

+[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png new file mode 100644 index 00000000..76cf5150 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.fits new file mode 100644 index 00000000..d449120b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.html new file mode 100644 index 00000000..6b21f4a0 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.png new file mode 100644 index 00000000..f0b72e41 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/OI145_CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/OI145_CII158.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.html new file mode 100644 index 00000000..bdc88365 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm/[C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm/[C II] 158 µm Intensity Ratio + +
+

+[O I] 145 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.png new file mode 100644 index 00000000..e7af45fa Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/OI145_OI63.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/OI145_OI63.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.html new file mode 100644 index 00000000..c3d3d721 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm/[O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 145 µm/[O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm/[O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.png new file mode 100644 index 00000000..afe5004e Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI145_OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits new file mode 100644 index 00000000..92981bc1 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.html new file mode 100644 index 00000000..d3acd0ee --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm + [C II] 158 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm + [C II] 158 µm Intensity + +
+

+[O I] 63 µm + [C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.png new file mode 100644 index 00000000..6d186566 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/OI63+CII158_FIR.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/OI63+CII158_FIR.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html new file mode 100644 index 00000000..f21bd9b7 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm + [C II] 158 µm/I<sub>FIR</sub> Intensity Ratio + +
+

+[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png new file mode 100644 index 00000000..8218796b Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63+CII158_FIR.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.fits new file mode 100644 index 00000000..290b93a6 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.fits differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.html new file mode 100644 index 00000000..6978f81e --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.png new file mode 100644 index 00000000..829d6983 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/OI63_CII158.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/OI63_CII158.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.html new file mode 100644 index 00000000..3e9f2381 --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm/[C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: kt2020

+
+
+
+
+
+
+
+ + [O I] 63 µm/[C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm/[C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. + +The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.png new file mode 100644 index 00000000..46fd3a0a Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/OI63_CII158.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/Ts.fits b/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.fits similarity index 100% rename from models/kt2020_Z1.0_non-clumpy_M0.0/Ts.fits rename to models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.fits diff --git a/models/kt2020_Z1.0_non-clumpy_M0.0/Ts.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.html similarity index 99% rename from models/kt2020_Z1.0_non-clumpy_M0.0/Ts.html rename to models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.html index 3b3c6950..fd0aabfb 100644 --- a/models/kt2020_Z1.0_non-clumpy_M0.0/Ts.html +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.html @@ -47,6 +47,7 @@

Surface Temperature emitted from the surface of a PDR as a function of the cloud density n and the FUV flux incident on the cloud G0. + The models in this ModelSet were created with the KOSMA-tau 2020 PDR code. The parameters were chosen to match as closely as possible those of the Wolfire-Kaufman 2020 models, so they may be more easily comparable. More details are in the FITS headers.

The FITS file is available for download. diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.png b/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.png new file mode 100644 index 00000000..27e3a5e9 Binary files /dev/null and b/models/kt2020_Z1.0_non-clumpy_M1000.0/Ts.png differ diff --git a/models/kt2020_Z1.0_non-clumpy_M1000.0/index.html b/models/kt2020_Z1.0_non-clumpy_M1000.0/index.html new file mode 100644 index 00000000..0fbaa2fd --- /dev/null +++ b/models/kt2020_Z1.0_non-clumpy_M1000.0/index.html @@ -0,0 +1,66 @@ + + + + + + + + + +
+
+ +

+KOSMA-tau 2020 models, computed to match closely the WK2020 models, non-clumpy, single clump 1000 M⊙, Z=1.0, losangle=0

+

+Below are links to the individual FITS files +and plots in the kt2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the kt2020 FITS and PNG files. + +

+ + + + + + + + + + + + + + + + +
[C I] 609 µm Intensity[C I] 370 µm Intensity[O I] 63 µm Intensity[O I] 145 µm Intensity
[C II] 158 µm IntensityCO(J=1-0) IntensityCO(J=2-1) IntensityCO(J=3-2) Intensity
CO(J=4-3) IntensityCO(J=5-4) IntensityCO(J=6-5) IntensityCO(J=7-6) Intensity
CO(J=8-7) IntensityCO(J=9-8) IntensityCO(J=10-9) IntensityCO(J=11-10) Intensity
CO(J=12-11) IntensityCO(J=13-12) IntensityCO(J=14-13) IntensityIFIR
[O I] 63 µm + [C II] 158 µm Intensity[O I] 145 µm + [C II] 158 µm IntensitySurface Temperature[O I] 145 µm/[O I] 63 µm Intensity Ratio
[O I] 145 µm/[C II] 158 µm Intensity Ratio[O I] 63 µm/[C II] 158 µm Intensity Ratio[C II] 158 µm/[C I] 609 µm Intensity Ratio[C I] 370 µm/[C I] 609 µm Intensity Ratio
[C II] 158 µm/CO(J=1-0) Intensity Ratio[C II] 158 µm/CO(J=2-1) Intensity Ratio[C II] 158 µm/CO(J=3-2) Intensity Ratio[C II] 158 µm/CO(J=4-3) Intensity Ratio
[C II] 158 µm/CO(J=5-4) Intensity Ratio[C II] 158 µm/CO(J=6-5) Intensity RatioCO(J=2-1)/CO(J=1-0) Intensity RatioCO(J=3-2)/CO(J=1-0) Intensity Ratio
CO(J=3-2)/CO(J=2-1) Intensity RatioCO(J=4-3)/CO(J=1-0) Intensity RatioCO(J=4-3)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=1-0) Intensity Ratio
CO(J=6-5)/CO(J=2-1) Intensity RatioCO(J=6-5)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=1-0) Intensity RatioCO(J=7-6)/CO(J=2-1) Intensity Ratio
CO(J=7-6)/CO(J=4-3) Intensity RatioCO(J=7-6)/CO(J=5-4) Intensity RatioCO(J=7-6)/CO(J=6-5) Intensity RatioCO(J=8-7)/CO(J=5-4) Intensity Ratio
CO(J=8-7)/CO(J=6-5) Intensity RatioCO(J=9-8)/CO(J=5-4) Intensity RatioCO(J=9-8)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=5-4) Intensity Ratio
CO(J=10-9)/CO(J=6-5) Intensity RatioCO(J=10-9)/CO(J=7-6) Intensity RatioCO(J=11-10)/CO(J=5-4) Intensity RatioCO(J=11-10)/CO(J=6-5) Intensity Ratio
CO(J=12-11)/CO(J=5-4) Intensity RatioCO(J=12-11)/CO(J=6-5) Intensity RatioCO(J=13-12)/CO(J=5-4) Intensity RatioCO(J=13-12)/CO(J=6-5) Intensity Ratio
CO(J=14-13)/CO(J=5-4) Intensity RatioCO(J=14-13)/CO(J=6-5) Intensity Ratio[O I] 63 µm + [C II] 158 µm/IFIR Intensity Ratio[O I] 145 µm + [C II] 158 µm/IFIR Intensity Ratio
+

+
+ + + + + diff --git a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.fits b/models/smc_Z0.1_constant_density/ciioifirwebsmccut.fits deleted file mode 100644 index b50c6283..00000000 --- a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.fits +++ /dev/null @@ -1,9 +0,0 @@ -SIMPLE = T / conforms to FITS standard BITPIX = -32 / array data type NAXIS = 2 / number of array dimensions NAXIS1 = 21 NAXIS2 = 23 CELLSCAL= 'CONSTANT' / DATAMIN = 1.21177265555E-06 / DATAMAX = 2.50240545720E-02 / HISTORY # HISTORY TITLE = '(CII+OI)/I FIR' HISTORY UNITS = ' ' HISTORY # HISTORY # / Models of Wolfire 2010 & Hollenbac h 2012, ApJ HISTORY # / Model Parameters: HISTORY VERSION = 1. HISTORY DVDOP = 1.5 / Turbulent Doppler Velocity (km/s) HISTORY ABUNDC = 3.19999999E-05 / Carbon Abundance (C/H) HISTORY ABUNDO = 6.39999998E-05 / Oxygen Abundance (O/H) HISTORY ABUNDSI = 3.40000014E-07 / Silicon Abundance (Si/H) HISTORY ABUNDS = 5.60000035E-06 / Sulfur Abundance (S/H) HISTORY ABUNDFE = 3.40000028E-08 / Iron Abundance (Fe/H) HISTORY ABUNDMG = 2.1999999E-07 / Magnesium Abundance (Mg/H) HISTORY ABUNDPA = 3.99999998E-08 / PAH Abundance (PAH/H) HISTORY ABUNDD = 0.200000003 / Dust Abundance wrt local ISM HISTORY AV = 10. / Optical Depth HISTORY ABUNDZ = 0.200000003 / Dust and Metals wrt local ISM HISTORY TAUV = 1.79999995 / Ratio of tau_UV/tau_V HISTORY HEAT = 'BTF' / Bakes & Tielens - Flat PAHs HISTORY FITS: Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 2016-08-12T14:24:34.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=ciioifirwebsmc.fits HISTORY FITS: out=ciioifirwebsmc.mir HISTORY FITS: op=xyin HISTORY IMSUB: Miriad Imsub: version 1.0 3-dec-02 HISTORY IMSUB: Executed on: 2016-08-12T14:24:38.0 HISTORY IMSUB: Command line inputs follow: HISTORY IMSUB: in=ciioifirwebsmc.mir HISTORY IMSUB: region=abspix,box(5,0,25,29) HISTORY IMSUB: out=test.mir HISTORY FITS: Miriad fits: fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 16AUG12:14:24:46.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=ciioifirwebsmc.mir HISTORY FITS: op=xyout HISTORY FITS: out=ciioifirwebsmccut.fits HISTORY FITS: in=test.mir HISTORY FITS: NOTE: Use options=varwt if loading into Miriad HISTORY FITS: Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 2016-08-16T15:12:22.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=ciioifirwebsmccut.fits HISTORY FITS: op=xyin HISTORY FITS: out=ciioifirwebsmccut.mir HISTORY IMSUB: Miriad Imsub: version 1.0 3-dec-02 HISTORY IMSUB: Executed on: 2016-08-16T15:12:32.0 HISTORY IMSUB: Command line inputs follow: HISTORY IMSUB: in=ciioifirwebsmccut.mir HISTORY IMSUB: out=tmp.mir HISTORY IMSUB: region=box(1,7,21,29) HISTORY FITS: Miriad fits: fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 16AUG16:15:13:05.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=tmp.mir HISTORY FITS: out=ciioifirwebsmccut.fits HISTORY FITS: op=xyout HISTORY FITS: NOTE: Use options=varwt if loading into Miriad ORIGIN = 'Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC' / BUNIT = '' BMAJ = BMIN = BPA = MODELTYP= 'ratio ' CUNIT1 = 'cm-3 ' / Units of coordinate increment and value CUNIT2 = 'Habing ' WCSAXES = 2 / Number of coordinate axes CRPIX1 = -3.0 / Pixel coordinate of reference point CRPIX2 = -5.0 / Pixel coordinate of reference point CDELT1 = 0.25 / [cm-3] Coordinate increment at reference point CDELT2 = 0.25 / Coordinate increment at reference point CTYPE1 = 'LOGN(/CM' / Coordinate type code CTYPE2 = 'LOGG_0' / Coordinate type code CRVAL1 = 1.0 / [cm-3] Coordinate value at reference point CRVAL2 = -0.5 / Coordinate value at reference point LATPOLE = 90.0 / [deg] Native latitude of celestial pole MJDREF = 0.0 / [d] MJD of fiducial time END < <[<"<3<><|4<<\0<&bu;g;b -:;x;1Ċ;R@;{;k7;;‘<T<9p;F;;< Z~n;t;;\; };NN;|,;Y/r8 mh8/R8b;8T8c8Im9%K9`99ۍ:u:dH:8C:;;C;Q;UD;M;>HK;+H;778)8h[U8x)8J89X9L9|9͏:S:V:U:;K;X;::ve:̊+7p]77#8(X8p8Uӝ8~89T9:9>9q: ul:z:s:: :i:::B7P[7Z77 8$~8n!88b_8{4J8B8C9+J9tJ9T:=:Ah:Q5:W:T:Jpe:=m:06H7 7Ip97.7$838d!8!}8_88O9e99ȝ9:2::E9T9/9Ⲵ6e9t6E6:7:77D8K8QN88H88Ǖ89J9x_9F99W9{9 8996 76NJ=6P16GC7-^77 E8^87Uf7828ɲ89i91Lk9>:9Dz9D9B@9=a'94,515g6:66Ԇe7(7eJ77l8\8E8y(88ݱ8;9808(8PZ8қ88%f \ No newline at end of file diff --git a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.html b/models/smc_Z0.1_constant_density/ciioifirwebsmccut.html deleted file mode 100644 index a86cd320..00000000 --- a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
-
- -

-([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio -

-

pdrtpy ModelSet: smc

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- - ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio - -
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-([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in the wk2006 Small Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers. -

-The FITS file is available for download. -

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- - - - - - - \ No newline at end of file diff --git a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.png b/models/smc_Z0.1_constant_density/ciioifirwebsmccut.png deleted file mode 100644 index 0a8982f6..00000000 Binary files a/models/smc_Z0.1_constant_density/ciioifirwebsmccut.png and /dev/null differ diff --git a/models/smc_Z0.1_constant_density/cpsmcwebcut.fits b/models/smc_Z0.1_constant_density/cpsmcwebcut.fits deleted file mode 100644 index 80fd18f7..00000000 Binary files a/models/smc_Z0.1_constant_density/cpsmcwebcut.fits and /dev/null differ diff --git a/models/smc_Z0.1_constant_density/cpsmcwebcut.html b/models/smc_Z0.1_constant_density/cpsmcwebcut.html deleted file mode 100644 index 49dd7c21..00000000 --- a/models/smc_Z0.1_constant_density/cpsmcwebcut.html +++ /dev/null @@ -1,65 +0,0 @@ - - - - - - -
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- -

-[C II] 158 µm Intensity -

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pdrtpy ModelSet: smc

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- - [C II] 158 µm Intensity - -
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-[C II] 158 µm Intensity emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in the wk2006 Small Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers. -

-The FITS file is available for download. -

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- - - - - - - \ No newline at end of file diff --git a/models/smc_Z0.1_constant_density/cpsmcwebcut.png b/models/smc_Z0.1_constant_density/cpsmcwebcut.png deleted file mode 100644 index f4c74612..00000000 Binary files a/models/smc_Z0.1_constant_density/cpsmcwebcut.png and /dev/null differ diff --git a/models/smc_Z0.1_constant_density/index.html b/models/smc_Z0.1_constant_density/index.html deleted file mode 100644 index 5f043200..00000000 --- a/models/smc_Z0.1_constant_density/index.html +++ /dev/null @@ -1,51 +0,0 @@ - - - - - - - - - -
-
- -

-Wolfire/Kaufman 2006 limited set of constant density models for Small Magellanic Cloud, Z=0.1

-

-Below are links to the individual FITS files -and plots in the smc ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. - - - -
[O I] 63 µm / [C II] 158 µm Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio[C II] 158 µm Intensity
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- - - - diff --git a/models/smc_Z0.1_constant_density/oicpsmcwebcut.fits b/models/smc_Z0.1_constant_density/oicpsmcwebcut.fits deleted file mode 100644 index be2a239c..00000000 --- a/models/smc_Z0.1_constant_density/oicpsmcwebcut.fits +++ /dev/null @@ -1,4 +0,0 @@ -SIMPLE = T / conforms to FITS standard BITPIX = -32 / array data type NAXIS = 2 / number of array dimensions NAXIS1 = 21 NAXIS2 = 23 CELLSCAL= 'CONSTANT' / DATAMIN = 3.99484559894E-02 / DATAMAX = 1.46709823608E+02 / HISTORY # HISTORY TITLE = '[O I] 63 Micron/[C II] 158 Micron' HISTORY UNITS = ' ' HISTORY # HISTORY # / Models of Wolfire 2010 and Hollenb ach 2012 HISTORY # / Model Parameters: HISTORY VERSION = 1. HISTORY DVDOP = 1.5 / Turbulent Doppler Velocity (km/s) HISTORY ABUNDC = 3.19999999E-05 / Carbon Abundance (C/H) HISTORY ABUNDO = 6.39999998E-05 / Oxygen Abundance (O/H) HISTORY ABUNDSI = 3.40000014E-07 / Silicon Abundance (Si/H) HISTORY ABUNDS = 5.60000035E-06 / Sulfur Abundance (S/H) HISTORY ABUNDFE = 3.40000028E-08 / Iron Abundance (Fe/H) HISTORY ABUNDMG = 2.1999999E-07 / Magnesium Abundance (Mg/H) HISTORY ABUNDPA = 3.99999998E-08 / PAH Abundance (PAH/H) HISTORY ABUNDD = 0.200000003 / Dust Abundance wrt local ISM HISTORY AV = 10. / Optical Depth HISTORY ABUNDZ = 0.200000003 / Dust and Metals wrt local ISM HISTORY TAUV = 1.79999995 / Ratio of tau_UV/tau_V HISTORY HEAT = 'BTF' / Bakes & Tielens - Flat PAHs HISTORY FITS: Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 2016-08-12T14:12:12.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=oicpwebsmc.fits HISTORY FITS: out=oicpwebsmc.mir HISTORY FITS: op=xyin HISTORY IMSUB: Miriad Imsub: version 1.0 3-dec-02 HISTORY IMSUB: Executed on: 2016-08-12T14:15:18.0 HISTORY IMSUB: Command line inputs follow: HISTORY IMSUB: in=oicpwebsmc.mir HISTORY IMSUB: region=abspix,box(5,0,25,29) HISTORY IMSUB: out=test.mir HISTORY FITS: Miriad fits: fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 16AUG12:14:19:19.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=test.mir HISTORY FITS: out=oicpsmcwebcut.fits HISTORY FITS: op=xyout HISTORY FITS: NOTE: Use options=varwt if loading into Miriad HISTORY FITS: Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 2016-08-16T15:08:01.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=oicpsmcwebcut.fits HISTORY FITS: out=oicpsmcwebcut.mir HISTORY FITS: op=xyin HISTORY IMSUB: Miriad Imsub: version 1.0 3-dec-02 HISTORY IMSUB: Executed on: 2016-08-16T15:09:37.0 HISTORY IMSUB: Command line inputs follow: HISTORY IMSUB: in=oicpsmcwebcut.mir HISTORY IMSUB: out=tmp.mir HISTORY IMSUB: region=box(1,7,21,29) HISTORY FITS: Miriad fits: fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC HISTORY FITS: Executed on: 16AUG16:15:11:48.0 HISTORY FITS: Command line inputs follow: HISTORY FITS: in=tmp.mir HISTORY FITS: out=oicpsmcwebcut.fits HISTORY FITS: op=xyout HISTORY FITS: NOTE: Use options=varwt if loading into Miriad ORIGIN = 'Miriad fits: CVS Revision 1.24, 2013/03/14 17:33:00 UTC' / BUNIT = '' BMAJ = BMIN = BPA = MODELTYP= 'ratio ' CUNIT1 = 'cm-3 ' / Units of coordinate increment and value CUNIT2 = 'Habing ' WCSAXES = 2 / Number of coordinate axes CRPIX1 = -3.0 / Pixel coordinate of reference point CRPIX2 = -5.0 / Pixel coordinate of reference point CDELT1 = 0.25 / [cm-3] Coordinate increment at reference point CDELT2 = 0.25 / Coordinate increment at reference point CTYPE1 = 'LOGN(/CM' / Coordinate type code CTYPE2 = 'LOGG_0' / Coordinate type code CRVAL1 = 1.0 / [cm-3] Coordinate value at reference point CRVAL2 = -0.5 / Coordinate value at reference point LATPOLE = 90.0 / [deg] Native latitude of celestial pole MJDREF = 0.0 / [d] MJD of fiducial time END =y==V=/C=#=.=W=c=R>9FK>/a? ?}?@N @dAA;AӪB! B&> -==X==X=0=>}>MNA>UU>j?G7?"@H@f@A#>EAEABG2`B_U>B>t=a=e=W=5>#2>lN>9?r?A`??+@*@@יA.A|AvBc0BI$>~(>G>%>t>><>?>? ?N?s?UU@@`@@#A?AA8BbBZ>!!>>c>UY>b>>?t?S??oZ@0@YX@6@ؿAA\9AV-BmB^8BeF>>>4>g>>G:>D>”??G9?[?Cy@ @_k@f@sQA\AC>An-AB$B_8>>p_>>??3?Z?O@@]5C@@qPA9AHAAAĴB$X -BrB?>>~Z>?"j?'?e[??@A@@цAIAK61A8A.AUB'BG{BBNH?&O??e?_?(?P??BR@z@m[@AA@W'AABBQC ??g?C^?{5?u?@&D@;\@i@ʢAA`OAArB?B^=B}B/BBlfCi?&?6N?[?V*??@a@RY@#@tA$ ArlABBPBp:B{BB֠BC?T?+E??E1?[@@+@kR@J@PA1ңAFAB bvB]BBƵBv8BBC ??+9?GAt]AsBBiBBB]BBhB⪬C{?E?u?k@)C@}@%S@Tɩ@k@A\ALcAAB6BpBBJB2BÆBC?B=@>@?@5yD@e3|@8@j@9@AAZAAܣMBA}Bw BB(lBjBŻB^!Bc@.@ke@)b*@Nc@@0 @"@@ٳA&`.AjAI%ABKB~ B\AHA<%B0BZ}BrBfBʽBB˼B<;Ba@;@/!4@N@z@Dz@[AxfAKA+AJZZABB6B`BqB3BRB,B*lB޲Bh@@5@WS@b@@A*AS>A|ATAUBB;QBeLBAABBB< - - - - - -
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- -

-[O I] 63 µm / [C II] 158 µm Intensity Ratio -

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pdrtpy ModelSet: smc

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- - [O I] 63 µm / [C II] 158 µm Intensity Ratio - -
-

-[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR -as a function of the cloud density n and the FUV flux incident on the cloud G0. -The models in the wk2006 Small Magellanic Cloud ModelSet are based Kaufman et al. 1999 and Kaufman et al. 2006 . They use these parameters. More details are in the FITS headers. -

-The FITS file is available for download. -

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- - - - - - - \ No newline at end of file diff --git a/models/smc_Z0.1_constant_density/oicpsmcwebcut.png b/models/smc_Z0.1_constant_density/oicpsmcwebcut.png deleted file mode 100644 index dc56ed7a..00000000 Binary files a/models/smc_Z0.1_constant_density/oicpsmcwebcut.png and /dev/null differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.fits new file mode 100644 index 00000000..b7f2270e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.html b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.html new file mode 100644 index 00000000..78caa994 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) / CO(J=1-0) Intensity Ratio + +
+

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.png b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.png new file mode 100644 index 00000000..e40e1947 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO10_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO10sm.fits b/models/smc_Z0.2_L0_constant_density/13CO10sm.fits new file mode 100644 index 00000000..c99fa369 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO10sm.html b/models/smc_Z0.2_L0_constant_density/13CO10sm.html new file mode 100644 index 00000000..f523767e --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) Intensity + +
+

+13CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO10sm.png b/models/smc_Z0.2_L0_constant_density/13CO10sm.png new file mode 100644 index 00000000..c9358ee3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.fits new file mode 100644 index 00000000..4c8a9695 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.html new file mode 100644 index 00000000..6d50baa0 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.png new file mode 100644 index 00000000..0f90ae3a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO21_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO21sm.fits new file mode 100644 index 00000000..c66085d9 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO21sm.html new file mode 100644 index 00000000..596cb660 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) Intensity + +
+

+13CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO21sm.png new file mode 100644 index 00000000..18753a96 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.fits b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.fits new file mode 100644 index 00000000..f5768819 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.html b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.html new file mode 100644 index 00000000..84c3625f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.png b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.png new file mode 100644 index 00000000..879b1d07 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32_13CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.fits new file mode 100644 index 00000000..45c122aa Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.html new file mode 100644 index 00000000..4331550e --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.png new file mode 100644 index 00000000..3dc80242 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32sm.fits b/models/smc_Z0.2_L0_constant_density/13CO32sm.fits new file mode 100644 index 00000000..90ec7beb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO32sm.html b/models/smc_Z0.2_L0_constant_density/13CO32sm.html new file mode 100644 index 00000000..c29c4ef2 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) Intensity + +
+

+13CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO32sm.png b/models/smc_Z0.2_L0_constant_density/13CO32sm.png new file mode 100644 index 00000000..059a29bb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO32sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.fits new file mode 100644 index 00000000..13f3645b Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.html new file mode 100644 index 00000000..43cbc34a --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.png new file mode 100644 index 00000000..b12201b3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.fits new file mode 100644 index 00000000..326fd830 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.html new file mode 100644 index 00000000..5757650b --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=5-4) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.png new file mode 100644 index 00000000..6c13e908 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO54_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.fits new file mode 100644 index 00000000..c10eea76 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.html new file mode 100644 index 00000000..5444bd27 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=6-5) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.png new file mode 100644 index 00000000..ac522b9c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO65_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.fits new file mode 100644 index 00000000..9dbf9ee2 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.html b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.html new file mode 100644 index 00000000..fef2ccf5 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.png b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.png new file mode 100644 index 00000000..82e5fffb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/13CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.fits b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.fits new file mode 100644 index 00000000..fa4e11f8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.html b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.html new file mode 100644 index 00000000..3f842a99 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm / [C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.png b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.png new file mode 100644 index 00000000..066fd6bc Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI370_CI609sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI370sm.fits b/models/smc_Z0.2_L0_constant_density/CI370sm.fits new file mode 100644 index 00000000..93df52e8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI370sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI370sm.html b/models/smc_Z0.2_L0_constant_density/CI370sm.html new file mode 100644 index 00000000..7345e669 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI370sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI370sm.png b/models/smc_Z0.2_L0_constant_density/CI370sm.png new file mode 100644 index 00000000..12c8ca09 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI370sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.fits new file mode 100644 index 00000000..5a32df74 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.html b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.html new file mode 100644 index 00000000..4201c64f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.png b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.png new file mode 100644 index 00000000..b1543d95 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.fits new file mode 100644 index 00000000..3e831c23 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.html b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.html new file mode 100644 index 00000000..138a5a69 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.png b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.png new file mode 100644 index 00000000..1eab6f4e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.fits new file mode 100644 index 00000000..88f49e58 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.html b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.html new file mode 100644 index 00000000..19d04cda --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=3-2) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.png b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.png new file mode 100644 index 00000000..66084dd6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_13CO32sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.fits new file mode 100644 index 00000000..b9be9eb1 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.html new file mode 100644 index 00000000..0f1e022d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.png new file mode 100644 index 00000000..377e4aac Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.fits new file mode 100644 index 00000000..40b72572 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.html b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.html new file mode 100644 index 00000000..f3b624b3 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.png b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.png new file mode 100644 index 00000000..a5669b1b Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.fits b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.fits new file mode 100644 index 00000000..8c2356e7 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.html b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.html new file mode 100644 index 00000000..3320b311 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=4-3) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.png b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.png new file mode 100644 index 00000000..55f4ec4c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609_CO43sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609sm.fits b/models/smc_Z0.2_L0_constant_density/CI609sm.fits new file mode 100644 index 00000000..a1605ce8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CI609sm.html b/models/smc_Z0.2_L0_constant_density/CI609sm.html new file mode 100644 index 00000000..6ad52f0d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CI609sm.png b/models/smc_Z0.2_L0_constant_density/CI609sm.png new file mode 100644 index 00000000..2ed6ba4f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CI609sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.fits new file mode 100644 index 00000000..d0c22410 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.html b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.html new file mode 100644 index 00000000..ca28eaec --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.png b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.png new file mode 100644 index 00000000..233ff522 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_13CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.fits new file mode 100644 index 00000000..3cec2303 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.html b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.html new file mode 100644 index 00000000..792f3c65 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.png b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.png new file mode 100644 index 00000000..eac8d42e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_13CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.fits new file mode 100644 index 00000000..73742e2d Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.html b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.html new file mode 100644 index 00000000..dbc58a40 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.png b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.png new file mode 100644 index 00000000..3f0299f1 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CI609sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.fits new file mode 100644 index 00000000..4dcfe578 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.html new file mode 100644 index 00000000..651abc14 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.png new file mode 100644 index 00000000..bd811d9e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.fits new file mode 100644 index 00000000..79a9f5f8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.html b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.html new file mode 100644 index 00000000..249772e8 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.png b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.png new file mode 100644 index 00000000..d893c687 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.fits new file mode 100644 index 00000000..baaa7bc4 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.html b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.html new file mode 100644 index 00000000..e721bca5 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.png b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.png new file mode 100644 index 00000000..607aad24 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO32sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.fits new file mode 100644 index 00000000..25d533bc Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.html new file mode 100644 index 00000000..ec544361 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.png new file mode 100644 index 00000000..1a411b16 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.fits b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.fits new file mode 100644 index 00000000..4646e39f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.html b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.html new file mode 100644 index 00000000..3a1c341a --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / I<sub>FIR</sub> Intensity Ratio + +
+

+[C II] 158 µm / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.png b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.png new file mode 100644 index 00000000..44547b96 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.fits b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.fits new file mode 100644 index 00000000..f6722f5b Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.html b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.html new file mode 100644 index 00000000..9d268010 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [O I] 145 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [O I] 145 µm Intensity Ratio + +
+

+[C II] 158 µm / [O I] 145 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.png b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.png new file mode 100644 index 00000000..ff9123f3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158_OI145sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158sm.fits b/models/smc_Z0.2_L0_constant_density/CII158sm.fits new file mode 100644 index 00000000..e50c5e80 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CII158sm.html b/models/smc_Z0.2_L0_constant_density/CII158sm.html new file mode 100644 index 00000000..fbda3a0f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CII158sm.png b/models/smc_Z0.2_L0_constant_density/CII158sm.png new file mode 100644 index 00000000..32a4bb40 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CII158sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.fits new file mode 100644 index 00000000..5a9767d6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.html new file mode 100644 index 00000000..a3db57a4 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.png new file mode 100644 index 00000000..3d8c728a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.fits new file mode 100644 index 00000000..139328d3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.html new file mode 100644 index 00000000..fde4306d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.png new file mode 100644 index 00000000..c1051ebd Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.fits b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.fits new file mode 100644 index 00000000..5670b834 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.html b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.html new file mode 100644 index 00000000..8112986f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.png b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.png new file mode 100644 index 00000000..d7888a69 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO109_CO76sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CO10sm.fits new file mode 100644 index 00000000..55e795ab Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO10sm.html b/models/smc_Z0.2_L0_constant_density/CO10sm.html new file mode 100644 index 00000000..67d5c004 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO10sm.png b/models/smc_Z0.2_L0_constant_density/CO10sm.png new file mode 100644 index 00000000..d747ec0a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.fits new file mode 100644 index 00000000..279eddfb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.html new file mode 100644 index 00000000..42e434bb --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.png new file mode 100644 index 00000000..e0c7d23a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.fits new file mode 100644 index 00000000..8a1eb74f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.html new file mode 100644 index 00000000..0b7e452e --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.png new file mode 100644 index 00000000..e4684652 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.fits b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.fits new file mode 100644 index 00000000..7c5e4a0e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.html b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.html new file mode 100644 index 00000000..e1db51ea --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=8-7) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=8-7) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=8-7) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.png b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.png new file mode 100644 index 00000000..d962271c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110_CO87sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110sm.fits b/models/smc_Z0.2_L0_constant_density/CO1110sm.fits new file mode 100644 index 00000000..61119cde Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1110sm.html b/models/smc_Z0.2_L0_constant_density/CO1110sm.html new file mode 100644 index 00000000..9fd0f946 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1110sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1110sm.png b/models/smc_Z0.2_L0_constant_density/CO1110sm.png new file mode 100644 index 00000000..a6a4cec7 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1110sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.fits new file mode 100644 index 00000000..d9f319ed Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.html new file mode 100644 index 00000000..5306989f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.png new file mode 100644 index 00000000..002ec9e2 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1211_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.fits new file mode 100644 index 00000000..9165bb43 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.html new file mode 100644 index 00000000..54055881 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.png new file mode 100644 index 00000000..e5e875c3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1211_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.fits new file mode 100644 index 00000000..c9bc106b Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.html new file mode 100644 index 00000000..83b2701c --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.png new file mode 100644 index 00000000..d50d800e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1312_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.fits new file mode 100644 index 00000000..806c5b4e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.html new file mode 100644 index 00000000..13c4f479 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.png new file mode 100644 index 00000000..f910b802 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1312_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.fits new file mode 100644 index 00000000..2faa93b2 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.html new file mode 100644 index 00000000..414203f0 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.png new file mode 100644 index 00000000..e0b54b1d Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1413_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.fits new file mode 100644 index 00000000..dc470ebb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.html new file mode 100644 index 00000000..915289d4 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.png new file mode 100644 index 00000000..8c355af6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1413_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.fits new file mode 100644 index 00000000..191904c1 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.html new file mode 100644 index 00000000..622548bb --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.png new file mode 100644 index 00000000..d0ca319b Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1514_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.fits new file mode 100644 index 00000000..87c9ce83 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.html new file mode 100644 index 00000000..bd32b1c0 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.png new file mode 100644 index 00000000..ced9fc36 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1514_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.fits new file mode 100644 index 00000000..4e726b78 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.html new file mode 100644 index 00000000..b5b01315 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.png new file mode 100644 index 00000000..cc261509 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1615_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.fits new file mode 100644 index 00000000..46eca5c3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.html new file mode 100644 index 00000000..d6dd28af --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.png new file mode 100644 index 00000000..670b7bf5 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1615_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.fits new file mode 100644 index 00000000..169cc664 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.html new file mode 100644 index 00000000..94998415 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.png new file mode 100644 index 00000000..a3a8ff85 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1716_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.fits new file mode 100644 index 00000000..d919bdbb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.html new file mode 100644 index 00000000..0d79e2e4 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.png new file mode 100644 index 00000000..218a8962 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1716_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.fits new file mode 100644 index 00000000..e3cc4d40 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.html new file mode 100644 index 00000000..d8e9006b --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.png new file mode 100644 index 00000000..1ce4e0fb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1817_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.fits new file mode 100644 index 00000000..b15037ac Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.html new file mode 100644 index 00000000..5946cf47 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.png new file mode 100644 index 00000000..cd6d51b6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO1817_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.fits new file mode 100644 index 00000000..60fa3017 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.html new file mode 100644 index 00000000..5f542f29 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.png new file mode 100644 index 00000000..e89a2e9a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO21_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CO21sm.fits new file mode 100644 index 00000000..e26eeed8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO21sm.html b/models/smc_Z0.2_L0_constant_density/CO21sm.html new file mode 100644 index 00000000..3ba13c3f --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO21sm.png b/models/smc_Z0.2_L0_constant_density/CO21sm.png new file mode 100644 index 00000000..c82ecff8 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.fits new file mode 100644 index 00000000..17400681 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.html new file mode 100644 index 00000000..112a3c2c --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.png new file mode 100644 index 00000000..8f8ee4c5 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.fits new file mode 100644 index 00000000..e3b14f64 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.html b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.html new file mode 100644 index 00000000..a788db64 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.png b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.png new file mode 100644 index 00000000..267e1e02 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32sm.fits b/models/smc_Z0.2_L0_constant_density/CO32sm.fits new file mode 100644 index 00000000..96a27fd4 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO32sm.html b/models/smc_Z0.2_L0_constant_density/CO32sm.html new file mode 100644 index 00000000..51ecdf14 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO32sm.png b/models/smc_Z0.2_L0_constant_density/CO32sm.png new file mode 100644 index 00000000..018569e0 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO32sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.fits new file mode 100644 index 00000000..d0f124f0 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.html b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.html new file mode 100644 index 00000000..47c9e4d9 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.png b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.png new file mode 100644 index 00000000..e23b3c90 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO43sm.fits b/models/smc_Z0.2_L0_constant_density/CO43sm.fits new file mode 100644 index 00000000..d1cb9a3f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO43sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO43sm.html b/models/smc_Z0.2_L0_constant_density/CO43sm.html new file mode 100644 index 00000000..18ac7429 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO43sm.png b/models/smc_Z0.2_L0_constant_density/CO43sm.png new file mode 100644 index 00000000..eea3537a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO43sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO54sm.fits new file mode 100644 index 00000000..d81f6c42 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO54sm.html new file mode 100644 index 00000000..154b7b65 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO54sm.png new file mode 100644 index 00000000..708fd2bc Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.fits new file mode 100644 index 00000000..4062ecd6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.html new file mode 100644 index 00000000..fc4e65c4 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.png new file mode 100644 index 00000000..c040e5e6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO65_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO65sm.fits new file mode 100644 index 00000000..c3dc14f7 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO65sm.html new file mode 100644 index 00000000..a81f3944 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO65sm.png new file mode 100644 index 00000000..5cf1f1cb Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.fits b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.fits new file mode 100644 index 00000000..077fb2fa Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.html b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.html new file mode 100644 index 00000000..c4f975fb --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.png b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.png new file mode 100644 index 00000000..427eea9a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO10sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.fits b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.fits new file mode 100644 index 00000000..a34f1707 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.html b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.html new file mode 100644 index 00000000..f3d2f5d7 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.png b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.png new file mode 100644 index 00000000..33ff8aaa Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.fits b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.fits new file mode 100644 index 00000000..09d39cd6 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.html b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.html new file mode 100644 index 00000000..f4820ad6 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.png b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.png new file mode 100644 index 00000000..f3f85239 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO43sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.fits new file mode 100644 index 00000000..a7dc832f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.html new file mode 100644 index 00000000..57814320 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.png new file mode 100644 index 00000000..281be0f9 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.fits new file mode 100644 index 00000000..93f8980d Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.html new file mode 100644 index 00000000..3a06914a --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.png new file mode 100644 index 00000000..b9140839 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76sm.fits b/models/smc_Z0.2_L0_constant_density/CO76sm.fits new file mode 100644 index 00000000..5d429580 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO76sm.html b/models/smc_Z0.2_L0_constant_density/CO76sm.html new file mode 100644 index 00000000..cbea5a36 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO76sm.png b/models/smc_Z0.2_L0_constant_density/CO76sm.png new file mode 100644 index 00000000..3964265a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO76sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.fits new file mode 100644 index 00000000..b7f835a7 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.html new file mode 100644 index 00000000..355a5944 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.png new file mode 100644 index 00000000..1d9adddf Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.fits new file mode 100644 index 00000000..60e1c833 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.html new file mode 100644 index 00000000..3ae4b073 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.png new file mode 100644 index 00000000..d4db5339 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87sm.fits b/models/smc_Z0.2_L0_constant_density/CO87sm.fits new file mode 100644 index 00000000..b886fa9c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO87sm.html b/models/smc_Z0.2_L0_constant_density/CO87sm.html new file mode 100644 index 00000000..22c9d3be --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO87sm.png b/models/smc_Z0.2_L0_constant_density/CO87sm.png new file mode 100644 index 00000000..e9d3c1a9 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO87sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.fits b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.fits new file mode 100644 index 00000000..1f8a96c2 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.html b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.html new file mode 100644 index 00000000..1502ec2a --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.png b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.png new file mode 100644 index 00000000..9ffa22fe Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO98_CO54sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.fits b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.fits new file mode 100644 index 00000000..f40c3797 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.html b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.html new file mode 100644 index 00000000..6733ffbd --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.png b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.png new file mode 100644 index 00000000..ec72efb9 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/CO98_CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S0sm.fits b/models/smc_Z0.2_L0_constant_density/H200S0sm.fits new file mode 100644 index 00000000..05919cf3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S0sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S0sm.html b/models/smc_Z0.2_L0_constant_density/H200S0sm.html new file mode 100644 index 00000000..37b25194 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(0) 28.2 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(0) 28.2 µm Intensity + +
+

+H20-0S(0) 28.2 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S0sm.png b/models/smc_Z0.2_L0_constant_density/H200S0sm.png new file mode 100644 index 00000000..72160939 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S0sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S1sm.fits b/models/smc_Z0.2_L0_constant_density/H200S1sm.fits new file mode 100644 index 00000000..1b54204e Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S1sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S1sm.html b/models/smc_Z0.2_L0_constant_density/H200S1sm.html new file mode 100644 index 00000000..f8d59b3d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(1) 17 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(1) 17 µm Intensity + +
+

+H20-0S(1) 17 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S1sm.png b/models/smc_Z0.2_L0_constant_density/H200S1sm.png new file mode 100644 index 00000000..7f144ce7 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S1sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.fits b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.fits new file mode 100644 index 00000000..a49f40d2 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.html b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.html new file mode 100644 index 00000000..3e2e0876 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.png b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.png new file mode 100644 index 00000000..5ce2e868 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2_H200S0sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.fits b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.fits new file mode 100644 index 00000000..f7142e4c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.html b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.html new file mode 100644 index 00000000..fd11b5f4 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.png b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.png new file mode 100644 index 00000000..39ca756f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2_H200S1sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2sm.fits b/models/smc_Z0.2_L0_constant_density/H200S2sm.fits new file mode 100644 index 00000000..f80e5299 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S2sm.html b/models/smc_Z0.2_L0_constant_density/H200S2sm.html new file mode 100644 index 00000000..113dc543 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm Intensity + +
+

+H20-0S(2) 12.3 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S2sm.png b/models/smc_Z0.2_L0_constant_density/H200S2sm.png new file mode 100644 index 00000000..86b18da3 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S2sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.fits b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.fits new file mode 100644 index 00000000..7c1a5820 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.html b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.html new file mode 100644 index 00000000..5798fa94 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.png b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.png new file mode 100644 index 00000000..36f60750 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S0sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.fits b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.fits new file mode 100644 index 00000000..3682c45a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.html b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.html new file mode 100644 index 00000000..3fa8b5c7 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.png b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.png new file mode 100644 index 00000000..a113adef Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S1sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.fits b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.fits new file mode 100644 index 00000000..1fb89cbc Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.html b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.html new file mode 100644 index 00000000..14eca835 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(2) 12.3 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.png b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.png new file mode 100644 index 00000000..3b952738 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3_H200S2sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3sm.fits b/models/smc_Z0.2_L0_constant_density/H200S3sm.fits new file mode 100644 index 00000000..0d098ccf Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H200S3sm.html b/models/smc_Z0.2_L0_constant_density/H200S3sm.html new file mode 100644 index 00000000..1652f503 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H200S3sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm Intensity + +
+

+H20-0S(3) 9.7 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H200S3sm.png b/models/smc_Z0.2_L0_constant_density/H200S3sm.png new file mode 100644 index 00000000..8496b650 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H200S3sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.fits b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.fits new file mode 100644 index 00000000..9095362d Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.html b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.html new file mode 100644 index 00000000..f19d4a61 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>2-1S(1) 2.24 µm / H<sub>2</sub>1-0S(1) 2.12 µm Intensity Ratio + +
+

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.png b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.png new file mode 100644 index 00000000..7aaf888d Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/H221S1_H210S1sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.fits b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.fits new file mode 100644 index 00000000..1cbcd361 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.html b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.html new file mode 100644 index 00000000..5c56e9dd --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 145 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.png b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.png new file mode 100644 index 00000000..3090d3d4 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.fits b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.fits new file mode 100644 index 00000000..155dda91 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.html b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.html new file mode 100644 index 00000000..20ccd43d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.png b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.png new file mode 100644 index 00000000..147d44dc Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145_13CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.fits b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.fits new file mode 100644 index 00000000..38bbe42c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.html b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.html new file mode 100644 index 00000000..8ab3f4e2 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / [O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / [O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm / [O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.png b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.png new file mode 100644 index 00000000..1fedb093 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145_OI63sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145sm.fits b/models/smc_Z0.2_L0_constant_density/OI145sm.fits new file mode 100644 index 00000000..ce2b79a1 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI145sm.html b/models/smc_Z0.2_L0_constant_density/OI145sm.html new file mode 100644 index 00000000..cd61394e --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI145sm.png b/models/smc_Z0.2_L0_constant_density/OI145sm.png new file mode 100644 index 00000000..789bcb50 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI145sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.fits b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.fits new file mode 100644 index 00000000..2cbeb92c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.html b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.html new file mode 100644 index 00000000..2c903d29 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.png b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.png new file mode 100644 index 00000000..17f3877a Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.fits b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.fits new file mode 100644 index 00000000..c9f0d38f Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.html b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.html new file mode 100644 index 00000000..2a6846cf --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.png b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.png new file mode 100644 index 00000000..e20e6151 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63_13CO65sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.fits b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.fits new file mode 100644 index 00000000..8f0d9062 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.html b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.html new file mode 100644 index 00000000..c1eed60d --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / [C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / [C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.png b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.png new file mode 100644 index 00000000..2712672c Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63_CII158sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63sm.fits b/models/smc_Z0.2_L0_constant_density/OI63sm.fits new file mode 100644 index 00000000..d3b16a78 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/OI63sm.html b/models/smc_Z0.2_L0_constant_density/OI63sm.html new file mode 100644 index 00000000..74b55f79 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/OI63sm.png b/models/smc_Z0.2_L0_constant_density/OI63sm.png new file mode 100644 index 00000000..be14de84 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/OI63sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.fits b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.fits new file mode 100644 index 00000000..e8e9e3c4 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.fits differ diff --git a/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.html b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.html new file mode 100644 index 00000000..ffbfe415 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+Temperature at AV = 0.01 +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + Temperature at A<sub>V</sub> = 0.01 + +
+

+Temperature at AV = 0.01 emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=0 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.png b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.png new file mode 100644 index 00000000..a44a6722 Binary files /dev/null and b/models/smc_Z0.2_L0_constant_density/TSAV0p01sm.png differ diff --git a/models/smc_Z0.2_L0_constant_density/index.html b/models/smc_Z0.2_L0_constant_density/index.html new file mode 100644 index 00000000..34f7da48 --- /dev/null +++ b/models/smc_Z0.2_L0_constant_density/index.html @@ -0,0 +1,73 @@ + + + + + + + + + +
+
+ +

+Wolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=0

+

+Below are links to the individual FITS files +and plots in the smc z=0.2 losangle=0 ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. + + + + + + + + + + + + + + + + + + + + + + + + + +
[O I] 63 µm / [C II] 158 µm Intensity Ratio[O I] 63 µm / 13CO(J=6-5) Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio
[O I] 145 µm / [O I] 63 µm Intensity Ratio[O I] 145 µm / 13CO(J=6-5) Intensity Ratio[C I] 370 µm / [C I] 609 µm Intensity Ratio[C II] 158 µm / [C I] 609 µm Intensity Ratio
[C II] 158 µm / [O I] 145 µm Intensity Ratio[C II] 158 µm / IFIR Intensity Ratio[C II] 158 µm / CO(J=1-0) Intensity Ratio[C II] 158 µm / CO(J=2-1) Intensity Ratio
[C II] 158 µm / CO(J=3-2) Intensity Ratio[C II] 158 µm / CO(J=6-5) Intensity Ratio[C II] 158 µm / 13CO(J=1-0) Intensity Ratio[C II] 158 µm / 13CO(J=6-5) Intensity Ratio
CO(J=2-1) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=4-3) Intensity Ratio
[C I] 609 µm / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=2-1) Intensity Ratio
[C I] 609 µm / 13CO(J=3-2) Intensity RatioCO(J=4-3) / CO(J=2-1) Intensity RatioCO(J=6-5) / CO(J=1-0) Intensity RatioCO(J=7-6) / CO(J=1-0) Intensity Ratio
CO(J=7-6) / CO(J=2-1) Intensity RatioCO(J=7-6) / CO(J=4-3) Intensity RatioCO(J=7-6) / CO(J=5-4) Intensity RatioCO(J=7-6) / CO(J=6-5) Intensity Ratio
CO(J=8-7) / CO(J=5-4) Intensity RatioCO(J=8-7) / CO(J=6-5) Intensity RatioCO(J=9-8) / CO(J=5-4) Intensity RatioCO(J=9-8) / CO(J=6-5) Intensity Ratio
CO(J=10-9) / CO(J=5-4) Intensity RatioCO(J=10-9) / CO(J=6-5) Intensity RatioCO(J=10-9) / CO(J=7-6) Intensity RatioCO(J=11-10) / CO(J=5-4) Intensity Ratio
CO(J=11-10) / CO(J=6-5) Intensity RatioCO(J=11-10) / CO(J=8-7) Intensity RatioCO(J=12-11) / CO(J=5-4) Intensity RatioCO(J=12-11) / CO(J=6-5) Intensity Ratio
CO(J=13-12) / CO(J=5-4) Intensity RatioCO(J=13-12) / CO(J=6-5) Intensity RatioCO(J=14-13) / CO(J=5-4) Intensity RatioCO(J=14-13) / CO(J=6-5) Intensity Ratio
CO(J=15-14) / CO(J=5-4) Intensity RatioCO(J=15-14) / CO(J=6-5) Intensity RatioCO(J=16-15) / CO(J=5-4) Intensity RatioCO(J=16-15) / CO(J=6-5) Intensity Ratio
CO(J=17-16) / CO(J=5-4) Intensity RatioCO(J=17-16) / CO(J=6-5) Intensity RatioCO(J=18-17) / CO(J=5-4) Intensity RatioCO(J=18-17) / CO(J=6-5) Intensity Ratio
13CO(J=1-0) / CO(J=1-0) Intensity Ratio13CO(J=2-1) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / CO(J=2-1) Intensity Ratio13CO(J=4-3) / CO(J=2-1) Intensity Ratio
13CO(J=5-4) / CO(J=2-1) Intensity Ratio13CO(J=6-5) / CO(J=2-1) Intensity Ratio13CO(J=7-6) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio
H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio
H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity RatioH22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio[C I] 370 µm Intensity[C I] 609 µm Intensity
[C II] 158 µm Intensity[O I] 63 µm Intensity[O I] 145 µm IntensityCO(J=1-0) Intensity
CO(J=2-1) IntensityCO(J=3-2) IntensityCO(J=4-3) IntensityCO(J=5-4) Intensity
CO(J=6-5) IntensityCO(J=7-6) IntensityCO(J=8-7) IntensityCO(J=11-10) Intensity
13CO(J=1-0) Intensity13CO(J=2-1) Intensity13CO(J=3-2) IntensityH20-0S(3) 9.7 µm Intensity
H20-0S(2) 12.3 µm IntensityH20-0S(1) 17 µm IntensityH20-0S(0) 28.2 µm IntensityTemperature at AV = 0.01
+

+
+
+ + + + diff --git a/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.fits new file mode 100644 index 00000000..b5f89077 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.html b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.html new file mode 100644 index 00000000..eaa58709 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) / CO(J=1-0) Intensity Ratio + +
+

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.png b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.png new file mode 100644 index 00000000..d732b1f7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO10_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO10sm.fits b/models/smc_Z0.2_L30_constant_density/13CO10sm.fits new file mode 100644 index 00000000..a47318ee Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO10sm.html b/models/smc_Z0.2_L30_constant_density/13CO10sm.html new file mode 100644 index 00000000..6ca2c9ce --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) Intensity + +
+

+13CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO10sm.png b/models/smc_Z0.2_L30_constant_density/13CO10sm.png new file mode 100644 index 00000000..ed277450 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.fits new file mode 100644 index 00000000..6ffb90b6 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.html new file mode 100644 index 00000000..d5c27ebb --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.png new file mode 100644 index 00000000..d7fdef04 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO21_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO21sm.fits new file mode 100644 index 00000000..eb1fff96 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO21sm.html new file mode 100644 index 00000000..76cdc025 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) Intensity + +
+

+13CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO21sm.png new file mode 100644 index 00000000..a7894b89 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.fits b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.fits new file mode 100644 index 00000000..3fc4b547 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.html b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.html new file mode 100644 index 00000000..25bd27d9 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.png b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.png new file mode 100644 index 00000000..ec5812fc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32_13CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.fits new file mode 100644 index 00000000..dc4dfd93 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.html new file mode 100644 index 00000000..10a2f909 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.png new file mode 100644 index 00000000..6070294c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32sm.fits b/models/smc_Z0.2_L30_constant_density/13CO32sm.fits new file mode 100644 index 00000000..3127c7d7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO32sm.html b/models/smc_Z0.2_L30_constant_density/13CO32sm.html new file mode 100644 index 00000000..38bb2cfa --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) Intensity + +
+

+13CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO32sm.png b/models/smc_Z0.2_L30_constant_density/13CO32sm.png new file mode 100644 index 00000000..94b2160d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO32sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.fits new file mode 100644 index 00000000..a845d12b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.html new file mode 100644 index 00000000..7d9b36e2 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.png new file mode 100644 index 00000000..21a06e5f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.fits new file mode 100644 index 00000000..7a034c2f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.html new file mode 100644 index 00000000..c1907b5a --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=5-4) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.png new file mode 100644 index 00000000..bbcb5c49 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO54_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.fits new file mode 100644 index 00000000..9cd14c92 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.html new file mode 100644 index 00000000..a2a0299b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=6-5) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.png new file mode 100644 index 00000000..18d26a93 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO65_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.fits new file mode 100644 index 00000000..ed8f8221 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.html b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.html new file mode 100644 index 00000000..bf9ffb07 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.png b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.png new file mode 100644 index 00000000..38d1b40b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/13CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.fits b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.fits new file mode 100644 index 00000000..0b016f62 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.html b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.html new file mode 100644 index 00000000..8e3674ca --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm / [C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.png b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.png new file mode 100644 index 00000000..87254110 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI370_CI609sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI370sm.fits b/models/smc_Z0.2_L30_constant_density/CI370sm.fits new file mode 100644 index 00000000..8b64303b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI370sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI370sm.html b/models/smc_Z0.2_L30_constant_density/CI370sm.html new file mode 100644 index 00000000..5a5b6c32 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI370sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI370sm.png b/models/smc_Z0.2_L30_constant_density/CI370sm.png new file mode 100644 index 00000000..1a050cd0 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI370sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.fits new file mode 100644 index 00000000..8bbb1cd1 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.html b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.html new file mode 100644 index 00000000..e7190e97 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.png b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.png new file mode 100644 index 00000000..6c51319f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.fits new file mode 100644 index 00000000..7579c35a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.html b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.html new file mode 100644 index 00000000..c41573d6 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.png b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.png new file mode 100644 index 00000000..d654f9ac Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.fits new file mode 100644 index 00000000..d80e2dcb Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.html b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.html new file mode 100644 index 00000000..3ed78233 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=3-2) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.png b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.png new file mode 100644 index 00000000..33bf8a93 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_13CO32sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.fits new file mode 100644 index 00000000..31bc640e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.html new file mode 100644 index 00000000..8e14e251 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.png new file mode 100644 index 00000000..bf0b1d62 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.fits new file mode 100644 index 00000000..0ee85b03 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.html b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.html new file mode 100644 index 00000000..4aefcd8b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.png b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.png new file mode 100644 index 00000000..99deec23 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.fits b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.fits new file mode 100644 index 00000000..b43a4114 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.html b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.html new file mode 100644 index 00000000..1b06d548 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=4-3) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.png b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.png new file mode 100644 index 00000000..29f66466 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609_CO43sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609sm.fits b/models/smc_Z0.2_L30_constant_density/CI609sm.fits new file mode 100644 index 00000000..42ab496c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CI609sm.html b/models/smc_Z0.2_L30_constant_density/CI609sm.html new file mode 100644 index 00000000..ee4a04d4 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CI609sm.png b/models/smc_Z0.2_L30_constant_density/CI609sm.png new file mode 100644 index 00000000..9bf2a0a6 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CI609sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.fits new file mode 100644 index 00000000..2ebe965e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.html b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.html new file mode 100644 index 00000000..944c9eb6 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.png b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.png new file mode 100644 index 00000000..7b1f0c03 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_13CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.fits new file mode 100644 index 00000000..8575e9b7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.html b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.html new file mode 100644 index 00000000..264278b0 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.png b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.png new file mode 100644 index 00000000..75fb3c39 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_13CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.fits new file mode 100644 index 00000000..db0792d8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.html b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.html new file mode 100644 index 00000000..62bfba5e --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.png b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.png new file mode 100644 index 00000000..ecdd64bc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CI609sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.fits new file mode 100644 index 00000000..250d1fab Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.html new file mode 100644 index 00000000..c1913679 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.png new file mode 100644 index 00000000..d244bfb8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.fits new file mode 100644 index 00000000..ff9c1586 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.html b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.html new file mode 100644 index 00000000..f7710cca --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.png b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.png new file mode 100644 index 00000000..443805f4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.fits new file mode 100644 index 00000000..40a3da33 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.html b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.html new file mode 100644 index 00000000..b43de5aa --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.png b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.png new file mode 100644 index 00000000..341a9894 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO32sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.fits new file mode 100644 index 00000000..d2b19aad Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.html new file mode 100644 index 00000000..0a33adbf --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.png new file mode 100644 index 00000000..5c264bc4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.fits b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.fits new file mode 100644 index 00000000..1bc9e278 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.html b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.html new file mode 100644 index 00000000..48baf8a8 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / I<sub>FIR</sub> Intensity Ratio + +
+

+[C II] 158 µm / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.png b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.png new file mode 100644 index 00000000..2ad085df Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.fits b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.fits new file mode 100644 index 00000000..8aade1b2 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.html b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.html new file mode 100644 index 00000000..8371bb4b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [O I] 145 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [O I] 145 µm Intensity Ratio + +
+

+[C II] 158 µm / [O I] 145 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.png b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.png new file mode 100644 index 00000000..65f9b2d3 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158_OI145sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158sm.fits b/models/smc_Z0.2_L30_constant_density/CII158sm.fits new file mode 100644 index 00000000..12a0ed69 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CII158sm.html b/models/smc_Z0.2_L30_constant_density/CII158sm.html new file mode 100644 index 00000000..63590592 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CII158sm.png b/models/smc_Z0.2_L30_constant_density/CII158sm.png new file mode 100644 index 00000000..6eb276a6 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CII158sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.fits new file mode 100644 index 00000000..7c17d9b6 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.html new file mode 100644 index 00000000..22681643 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.png new file mode 100644 index 00000000..53976f6e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.fits new file mode 100644 index 00000000..08deea83 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.html new file mode 100644 index 00000000..84be1347 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.png new file mode 100644 index 00000000..01485b23 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.fits b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.fits new file mode 100644 index 00000000..7e7372c8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.html b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.html new file mode 100644 index 00000000..d222097f --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.png b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.png new file mode 100644 index 00000000..a1e2d397 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO109_CO76sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CO10sm.fits new file mode 100644 index 00000000..36a24891 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO10sm.html b/models/smc_Z0.2_L30_constant_density/CO10sm.html new file mode 100644 index 00000000..3d051044 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO10sm.png b/models/smc_Z0.2_L30_constant_density/CO10sm.png new file mode 100644 index 00000000..85ed9f58 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.fits new file mode 100644 index 00000000..1c224463 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.html new file mode 100644 index 00000000..2ba5ea1e --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.png new file mode 100644 index 00000000..a370746e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.fits new file mode 100644 index 00000000..b2ea7135 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.html new file mode 100644 index 00000000..fd2ed3c8 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.png new file mode 100644 index 00000000..742cf5cb Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.fits b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.fits new file mode 100644 index 00000000..adb99880 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.html b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.html new file mode 100644 index 00000000..e04f799b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=8-7) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=8-7) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=8-7) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.png b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.png new file mode 100644 index 00000000..c2e3330d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110_CO87sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110sm.fits b/models/smc_Z0.2_L30_constant_density/CO1110sm.fits new file mode 100644 index 00000000..f7e860b7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1110sm.html b/models/smc_Z0.2_L30_constant_density/CO1110sm.html new file mode 100644 index 00000000..159e0d2b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1110sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1110sm.png b/models/smc_Z0.2_L30_constant_density/CO1110sm.png new file mode 100644 index 00000000..e8fc6ecc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1110sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.fits new file mode 100644 index 00000000..d5bdf42a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.html new file mode 100644 index 00000000..96556c13 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.png new file mode 100644 index 00000000..bd0aa7c7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1211_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.fits new file mode 100644 index 00000000..29ae7e1f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.html new file mode 100644 index 00000000..c8e9943b --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.png new file mode 100644 index 00000000..4133f0e8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1211_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.fits new file mode 100644 index 00000000..645ec58a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.html new file mode 100644 index 00000000..7e0554a1 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.png new file mode 100644 index 00000000..2425b91c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1312_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.fits new file mode 100644 index 00000000..ba15e073 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.html new file mode 100644 index 00000000..dde97379 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.png new file mode 100644 index 00000000..2feebfa0 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1312_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.fits new file mode 100644 index 00000000..ed49c571 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.html new file mode 100644 index 00000000..ee285b2d --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.png new file mode 100644 index 00000000..cc27b626 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1413_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.fits new file mode 100644 index 00000000..91fcb976 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.html new file mode 100644 index 00000000..8e9ebc72 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.png new file mode 100644 index 00000000..83a17ebc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1413_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.fits new file mode 100644 index 00000000..dec0ef0e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.html new file mode 100644 index 00000000..1c650438 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.png new file mode 100644 index 00000000..f9167973 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1514_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.fits new file mode 100644 index 00000000..803c37b4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.html new file mode 100644 index 00000000..400391e3 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.png new file mode 100644 index 00000000..0de01f2a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1514_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.fits new file mode 100644 index 00000000..a25a691c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.html new file mode 100644 index 00000000..3d10872d --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.png new file mode 100644 index 00000000..26babc19 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1615_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.fits new file mode 100644 index 00000000..2bece982 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.html new file mode 100644 index 00000000..534e5ee9 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.png new file mode 100644 index 00000000..af0804c7 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1615_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.fits new file mode 100644 index 00000000..0b094975 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.html new file mode 100644 index 00000000..981942e2 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.png new file mode 100644 index 00000000..8bcff78e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1716_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.fits new file mode 100644 index 00000000..807d13ea Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.html new file mode 100644 index 00000000..35f3dac1 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.png new file mode 100644 index 00000000..b2544f1b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1716_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.fits new file mode 100644 index 00000000..bc18afa2 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.html new file mode 100644 index 00000000..b3d7770f --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.png new file mode 100644 index 00000000..df47523a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1817_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.fits new file mode 100644 index 00000000..4ec0dd4d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.html new file mode 100644 index 00000000..d8032ad1 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.png new file mode 100644 index 00000000..2672ec84 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO1817_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.fits new file mode 100644 index 00000000..f335e8eb Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.html new file mode 100644 index 00000000..27a18818 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.png new file mode 100644 index 00000000..410a2b0e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO21_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CO21sm.fits new file mode 100644 index 00000000..49f75f6f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO21sm.html b/models/smc_Z0.2_L30_constant_density/CO21sm.html new file mode 100644 index 00000000..35e41d5c --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO21sm.png b/models/smc_Z0.2_L30_constant_density/CO21sm.png new file mode 100644 index 00000000..e2ed3cae Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.fits new file mode 100644 index 00000000..e5c4d020 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.html new file mode 100644 index 00000000..80e2abe8 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.png new file mode 100644 index 00000000..0d093c8c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.fits new file mode 100644 index 00000000..28fd191d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.html b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.html new file mode 100644 index 00000000..9c5650db --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.png b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.png new file mode 100644 index 00000000..a6e54320 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32sm.fits b/models/smc_Z0.2_L30_constant_density/CO32sm.fits new file mode 100644 index 00000000..afdd53c8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO32sm.html b/models/smc_Z0.2_L30_constant_density/CO32sm.html new file mode 100644 index 00000000..b5cb1003 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO32sm.png b/models/smc_Z0.2_L30_constant_density/CO32sm.png new file mode 100644 index 00000000..06eb9be0 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO32sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.fits new file mode 100644 index 00000000..10bfc5c3 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.html b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.html new file mode 100644 index 00000000..b73ca8c8 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.png b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.png new file mode 100644 index 00000000..fc8dfbfc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO43sm.fits b/models/smc_Z0.2_L30_constant_density/CO43sm.fits new file mode 100644 index 00000000..0967199c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO43sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO43sm.html b/models/smc_Z0.2_L30_constant_density/CO43sm.html new file mode 100644 index 00000000..618c50b7 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO43sm.png b/models/smc_Z0.2_L30_constant_density/CO43sm.png new file mode 100644 index 00000000..a2fadc09 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO43sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO54sm.fits new file mode 100644 index 00000000..183bae2d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO54sm.html new file mode 100644 index 00000000..7a9711d1 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO54sm.png new file mode 100644 index 00000000..a6728ceb Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.fits new file mode 100644 index 00000000..990f5c72 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.html new file mode 100644 index 00000000..45b76a10 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.png new file mode 100644 index 00000000..36c15c85 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO65_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO65sm.fits new file mode 100644 index 00000000..dc480921 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO65sm.html new file mode 100644 index 00000000..686bf769 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO65sm.png new file mode 100644 index 00000000..def2c99b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.fits b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.fits new file mode 100644 index 00000000..591ab05b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.html b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.html new file mode 100644 index 00000000..1582566c --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.png b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.png new file mode 100644 index 00000000..09f4a947 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO10sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.fits b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.fits new file mode 100644 index 00000000..627912bd Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.html b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.html new file mode 100644 index 00000000..b50fd73d --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.png b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.png new file mode 100644 index 00000000..25c97b28 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.fits b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.fits new file mode 100644 index 00000000..b8cb7b03 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.html b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.html new file mode 100644 index 00000000..a299c29a --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.png b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.png new file mode 100644 index 00000000..76161cdd Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO43sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.fits new file mode 100644 index 00000000..35afff60 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.html new file mode 100644 index 00000000..bdfc7451 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.png new file mode 100644 index 00000000..b1be8d19 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.fits new file mode 100644 index 00000000..c5564047 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.html new file mode 100644 index 00000000..363714ca --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.png new file mode 100644 index 00000000..482f6194 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76sm.fits b/models/smc_Z0.2_L30_constant_density/CO76sm.fits new file mode 100644 index 00000000..54839019 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO76sm.html b/models/smc_Z0.2_L30_constant_density/CO76sm.html new file mode 100644 index 00000000..9bfbc5c7 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO76sm.png b/models/smc_Z0.2_L30_constant_density/CO76sm.png new file mode 100644 index 00000000..5fd402dd Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO76sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.fits new file mode 100644 index 00000000..a1ae996e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.html new file mode 100644 index 00000000..8d5af46d --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.png new file mode 100644 index 00000000..9a5b6e53 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.fits new file mode 100644 index 00000000..8a92de3b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.html new file mode 100644 index 00000000..be8b3a17 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.png new file mode 100644 index 00000000..67004a62 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87sm.fits b/models/smc_Z0.2_L30_constant_density/CO87sm.fits new file mode 100644 index 00000000..cac7c650 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO87sm.html b/models/smc_Z0.2_L30_constant_density/CO87sm.html new file mode 100644 index 00000000..57892d0e --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO87sm.png b/models/smc_Z0.2_L30_constant_density/CO87sm.png new file mode 100644 index 00000000..3d050503 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO87sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.fits b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.fits new file mode 100644 index 00000000..2c495c92 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.html b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.html new file mode 100644 index 00000000..ce00d119 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.png b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.png new file mode 100644 index 00000000..e5892066 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO98_CO54sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.fits b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.fits new file mode 100644 index 00000000..a6058190 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.html b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.html new file mode 100644 index 00000000..9791a0c0 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.png b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.png new file mode 100644 index 00000000..87b0492a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/CO98_CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S0sm.fits b/models/smc_Z0.2_L30_constant_density/H200S0sm.fits new file mode 100644 index 00000000..5d894fd8 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S0sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S0sm.html b/models/smc_Z0.2_L30_constant_density/H200S0sm.html new file mode 100644 index 00000000..0aaa9aad --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(0) 28.2 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(0) 28.2 µm Intensity + +
+

+H20-0S(0) 28.2 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S0sm.png b/models/smc_Z0.2_L30_constant_density/H200S0sm.png new file mode 100644 index 00000000..8d9accc4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S0sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S1sm.fits b/models/smc_Z0.2_L30_constant_density/H200S1sm.fits new file mode 100644 index 00000000..065a674e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S1sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S1sm.html b/models/smc_Z0.2_L30_constant_density/H200S1sm.html new file mode 100644 index 00000000..e4068131 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(1) 17 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(1) 17 µm Intensity + +
+

+H20-0S(1) 17 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S1sm.png b/models/smc_Z0.2_L30_constant_density/H200S1sm.png new file mode 100644 index 00000000..cff4bba1 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S1sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.fits b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.fits new file mode 100644 index 00000000..e6f2a5ca Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.html b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.html new file mode 100644 index 00000000..91d964e5 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.png b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.png new file mode 100644 index 00000000..8d423d2d Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2_H200S0sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.fits b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.fits new file mode 100644 index 00000000..6c322470 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.html b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.html new file mode 100644 index 00000000..8518d752 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.png b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.png new file mode 100644 index 00000000..d032d8de Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2_H200S1sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2sm.fits b/models/smc_Z0.2_L30_constant_density/H200S2sm.fits new file mode 100644 index 00000000..e4272def Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S2sm.html b/models/smc_Z0.2_L30_constant_density/H200S2sm.html new file mode 100644 index 00000000..cda23750 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm Intensity + +
+

+H20-0S(2) 12.3 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S2sm.png b/models/smc_Z0.2_L30_constant_density/H200S2sm.png new file mode 100644 index 00000000..7a4f212e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S2sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.fits b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.fits new file mode 100644 index 00000000..aed69f24 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.html b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.html new file mode 100644 index 00000000..9003e44a --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.png b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.png new file mode 100644 index 00000000..ad9a1f59 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S0sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.fits b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.fits new file mode 100644 index 00000000..90ebe89c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.html b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.html new file mode 100644 index 00000000..f218c815 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.png b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.png new file mode 100644 index 00000000..e475e7dd Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S1sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.fits b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.fits new file mode 100644 index 00000000..5d2f3bd2 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.html b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.html new file mode 100644 index 00000000..6a1c30f2 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(2) 12.3 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.png b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.png new file mode 100644 index 00000000..cbd89c1c Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3_H200S2sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3sm.fits b/models/smc_Z0.2_L30_constant_density/H200S3sm.fits new file mode 100644 index 00000000..8fc7b09e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H200S3sm.html b/models/smc_Z0.2_L30_constant_density/H200S3sm.html new file mode 100644 index 00000000..9f1b2d7c --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H200S3sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm Intensity + +
+

+H20-0S(3) 9.7 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H200S3sm.png b/models/smc_Z0.2_L30_constant_density/H200S3sm.png new file mode 100644 index 00000000..e8bb692b Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H200S3sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.fits b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.fits new file mode 100644 index 00000000..a07990ef Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.html b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.html new file mode 100644 index 00000000..c1ecbe60 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>2-1S(1) 2.24 µm / H<sub>2</sub>1-0S(1) 2.12 µm Intensity Ratio + +
+

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.png b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.png new file mode 100644 index 00000000..2c53d0c4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/H221S1_H210S1sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.fits b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.fits new file mode 100644 index 00000000..23146161 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.html b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.html new file mode 100644 index 00000000..fc0989d0 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 145 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.png b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.png new file mode 100644 index 00000000..f1d2f156 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.fits b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.fits new file mode 100644 index 00000000..a0075fcc Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.html b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.html new file mode 100644 index 00000000..b71900cb --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.png b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.png new file mode 100644 index 00000000..9c245546 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145_13CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.fits b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.fits new file mode 100644 index 00000000..c0e1ed9e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.html b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.html new file mode 100644 index 00000000..1004ff48 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / [O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / [O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm / [O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.png b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.png new file mode 100644 index 00000000..b8453710 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145_OI63sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145sm.fits b/models/smc_Z0.2_L30_constant_density/OI145sm.fits new file mode 100644 index 00000000..c4ee5fbb Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI145sm.html b/models/smc_Z0.2_L30_constant_density/OI145sm.html new file mode 100644 index 00000000..d4d5f8a1 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI145sm.png b/models/smc_Z0.2_L30_constant_density/OI145sm.png new file mode 100644 index 00000000..2d7e9026 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI145sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.fits b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.fits new file mode 100644 index 00000000..35216775 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.html b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.html new file mode 100644 index 00000000..fe93d4e3 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.png b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.png new file mode 100644 index 00000000..94bc520e Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.fits b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.fits new file mode 100644 index 00000000..e8e8a36a Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.html b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.html new file mode 100644 index 00000000..cbe97ed5 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.png b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.png new file mode 100644 index 00000000..fb17098f Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63_13CO65sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.fits b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.fits new file mode 100644 index 00000000..e5637962 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.html b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.html new file mode 100644 index 00000000..1e6e6eb4 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / [C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / [C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.png b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.png new file mode 100644 index 00000000..d2eb5134 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63_CII158sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63sm.fits b/models/smc_Z0.2_L30_constant_density/OI63sm.fits new file mode 100644 index 00000000..b42a4414 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/OI63sm.html b/models/smc_Z0.2_L30_constant_density/OI63sm.html new file mode 100644 index 00000000..e130eba9 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/OI63sm.png b/models/smc_Z0.2_L30_constant_density/OI63sm.png new file mode 100644 index 00000000..dc4c4622 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/OI63sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.fits b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.fits new file mode 100644 index 00000000..e8e9e3c4 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.fits differ diff --git a/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.html b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.html new file mode 100644 index 00000000..39adcb94 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+Temperature at AV = 0.01 +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + Temperature at A<sub>V</sub> = 0.01 + +
+

+Temperature at AV = 0.01 emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=30 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.png b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.png new file mode 100644 index 00000000..a44a6722 Binary files /dev/null and b/models/smc_Z0.2_L30_constant_density/TSAV0p01sm.png differ diff --git a/models/smc_Z0.2_L30_constant_density/index.html b/models/smc_Z0.2_L30_constant_density/index.html new file mode 100644 index 00000000..a52df0d5 --- /dev/null +++ b/models/smc_Z0.2_L30_constant_density/index.html @@ -0,0 +1,73 @@ + + + + + + + + + +
+
+ +

+Wolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=30

+

+Below are links to the individual FITS files +and plots in the smc z=0.2 losangle=30 ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. + + + + + + + + + + + + + + + + + + + + + + + + + +
[O I] 63 µm / [C II] 158 µm Intensity Ratio[O I] 63 µm / 13CO(J=6-5) Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio
[O I] 145 µm / [O I] 63 µm Intensity Ratio[O I] 145 µm / 13CO(J=6-5) Intensity Ratio[C I] 370 µm / [C I] 609 µm Intensity Ratio[C II] 158 µm / [C I] 609 µm Intensity Ratio
[C II] 158 µm / [O I] 145 µm Intensity Ratio[C II] 158 µm / IFIR Intensity Ratio[C II] 158 µm / CO(J=1-0) Intensity Ratio[C II] 158 µm / CO(J=2-1) Intensity Ratio
[C II] 158 µm / CO(J=3-2) Intensity Ratio[C II] 158 µm / CO(J=6-5) Intensity Ratio[C II] 158 µm / 13CO(J=1-0) Intensity Ratio[C II] 158 µm / 13CO(J=6-5) Intensity Ratio
CO(J=2-1) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=4-3) Intensity Ratio
[C I] 609 µm / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=2-1) Intensity Ratio
[C I] 609 µm / 13CO(J=3-2) Intensity RatioCO(J=4-3) / CO(J=2-1) Intensity RatioCO(J=6-5) / CO(J=1-0) Intensity RatioCO(J=7-6) / CO(J=1-0) Intensity Ratio
CO(J=7-6) / CO(J=2-1) Intensity RatioCO(J=7-6) / CO(J=4-3) Intensity RatioCO(J=7-6) / CO(J=5-4) Intensity RatioCO(J=7-6) / CO(J=6-5) Intensity Ratio
CO(J=8-7) / CO(J=5-4) Intensity RatioCO(J=8-7) / CO(J=6-5) Intensity RatioCO(J=9-8) / CO(J=5-4) Intensity RatioCO(J=9-8) / CO(J=6-5) Intensity Ratio
CO(J=10-9) / CO(J=5-4) Intensity RatioCO(J=10-9) / CO(J=6-5) Intensity RatioCO(J=10-9) / CO(J=7-6) Intensity RatioCO(J=11-10) / CO(J=5-4) Intensity Ratio
CO(J=11-10) / CO(J=6-5) Intensity RatioCO(J=11-10) / CO(J=8-7) Intensity RatioCO(J=12-11) / CO(J=5-4) Intensity RatioCO(J=12-11) / CO(J=6-5) Intensity Ratio
CO(J=13-12) / CO(J=5-4) Intensity RatioCO(J=13-12) / CO(J=6-5) Intensity RatioCO(J=14-13) / CO(J=5-4) Intensity RatioCO(J=14-13) / CO(J=6-5) Intensity Ratio
CO(J=15-14) / CO(J=5-4) Intensity RatioCO(J=15-14) / CO(J=6-5) Intensity RatioCO(J=16-15) / CO(J=5-4) Intensity RatioCO(J=16-15) / CO(J=6-5) Intensity Ratio
CO(J=17-16) / CO(J=5-4) Intensity RatioCO(J=17-16) / CO(J=6-5) Intensity RatioCO(J=18-17) / CO(J=5-4) Intensity RatioCO(J=18-17) / CO(J=6-5) Intensity Ratio
13CO(J=1-0) / CO(J=1-0) Intensity Ratio13CO(J=2-1) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / CO(J=2-1) Intensity Ratio13CO(J=4-3) / CO(J=2-1) Intensity Ratio
13CO(J=5-4) / CO(J=2-1) Intensity Ratio13CO(J=6-5) / CO(J=2-1) Intensity Ratio13CO(J=7-6) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio
H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio
H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity RatioH22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio[C I] 370 µm Intensity[C I] 609 µm Intensity
[C II] 158 µm Intensity[O I] 63 µm Intensity[O I] 145 µm IntensityCO(J=1-0) Intensity
CO(J=2-1) IntensityCO(J=3-2) IntensityCO(J=4-3) IntensityCO(J=5-4) Intensity
CO(J=6-5) IntensityCO(J=7-6) IntensityCO(J=8-7) IntensityCO(J=11-10) Intensity
13CO(J=1-0) Intensity13CO(J=2-1) Intensity13CO(J=3-2) IntensityH20-0S(3) 9.7 µm Intensity
H20-0S(2) 12.3 µm IntensityH20-0S(1) 17 µm IntensityH20-0S(0) 28.2 µm IntensityTemperature at AV = 0.01
+

+
+
+ + + + diff --git a/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.fits new file mode 100644 index 00000000..702a58a9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.html b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.html new file mode 100644 index 00000000..d44155dc --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) / CO(J=1-0) Intensity Ratio + +
+

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.png b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.png new file mode 100644 index 00000000..f23cf565 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO10_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO10sm.fits b/models/smc_Z0.2_L45_constant_density/13CO10sm.fits new file mode 100644 index 00000000..57f6640f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO10sm.html b/models/smc_Z0.2_L45_constant_density/13CO10sm.html new file mode 100644 index 00000000..5703820c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) Intensity + +
+

+13CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO10sm.png b/models/smc_Z0.2_L45_constant_density/13CO10sm.png new file mode 100644 index 00000000..8d0ba985 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.fits new file mode 100644 index 00000000..8c56312b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.html new file mode 100644 index 00000000..8566d612 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.png new file mode 100644 index 00000000..828880be Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO21_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO21sm.fits new file mode 100644 index 00000000..1f9f9d18 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO21sm.html new file mode 100644 index 00000000..29260578 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) Intensity + +
+

+13CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO21sm.png new file mode 100644 index 00000000..f6d9ba9a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.fits b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.fits new file mode 100644 index 00000000..14454465 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.html b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.html new file mode 100644 index 00000000..36d5f94b --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.png b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.png new file mode 100644 index 00000000..06cd71c9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32_13CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.fits new file mode 100644 index 00000000..3ed6d0b3 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.html new file mode 100644 index 00000000..36825352 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.png new file mode 100644 index 00000000..563a21b8 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32sm.fits b/models/smc_Z0.2_L45_constant_density/13CO32sm.fits new file mode 100644 index 00000000..65d27419 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO32sm.html b/models/smc_Z0.2_L45_constant_density/13CO32sm.html new file mode 100644 index 00000000..31ec011e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) Intensity + +
+

+13CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO32sm.png b/models/smc_Z0.2_L45_constant_density/13CO32sm.png new file mode 100644 index 00000000..cf7018cb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO32sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.fits new file mode 100644 index 00000000..94e195d8 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.html new file mode 100644 index 00000000..a137f76e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.png new file mode 100644 index 00000000..d5f31f6c Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.fits new file mode 100644 index 00000000..38c91a1f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.html new file mode 100644 index 00000000..82823c1c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=5-4) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.png new file mode 100644 index 00000000..eb2c4b4f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO54_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.fits new file mode 100644 index 00000000..96b25703 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.html new file mode 100644 index 00000000..ac7131c7 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=6-5) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.png new file mode 100644 index 00000000..2d8e1da2 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO65_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.fits new file mode 100644 index 00000000..496a5336 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.html b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.html new file mode 100644 index 00000000..4c64959e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.png b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.png new file mode 100644 index 00000000..3e791027 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/13CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.fits b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.fits new file mode 100644 index 00000000..df0f934f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.html b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.html new file mode 100644 index 00000000..25931afa --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm / [C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.png b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.png new file mode 100644 index 00000000..6ef4da7e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI370_CI609sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI370sm.fits b/models/smc_Z0.2_L45_constant_density/CI370sm.fits new file mode 100644 index 00000000..381a6d9b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI370sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI370sm.html b/models/smc_Z0.2_L45_constant_density/CI370sm.html new file mode 100644 index 00000000..8f3e75de --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI370sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI370sm.png b/models/smc_Z0.2_L45_constant_density/CI370sm.png new file mode 100644 index 00000000..fa330beb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI370sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.fits new file mode 100644 index 00000000..dc52524d Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.html b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.html new file mode 100644 index 00000000..2c6f3216 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.png b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.png new file mode 100644 index 00000000..1feb51b1 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.fits new file mode 100644 index 00000000..fa705286 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.html b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.html new file mode 100644 index 00000000..62018fdb --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.png b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.png new file mode 100644 index 00000000..14678764 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.fits new file mode 100644 index 00000000..344676a9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.html b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.html new file mode 100644 index 00000000..834c8bf1 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=3-2) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.png b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.png new file mode 100644 index 00000000..6aef1bf5 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_13CO32sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.fits new file mode 100644 index 00000000..d070242f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.html new file mode 100644 index 00000000..78c9c07f --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.png new file mode 100644 index 00000000..1aaa7301 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.fits new file mode 100644 index 00000000..41dd8ad9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.html b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.html new file mode 100644 index 00000000..6c613892 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.png b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.png new file mode 100644 index 00000000..1019056d Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.fits b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.fits new file mode 100644 index 00000000..31ce2425 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.html b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.html new file mode 100644 index 00000000..6fac4aba --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=4-3) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.png b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.png new file mode 100644 index 00000000..dc26b5f9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609_CO43sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609sm.fits b/models/smc_Z0.2_L45_constant_density/CI609sm.fits new file mode 100644 index 00000000..db372ac9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CI609sm.html b/models/smc_Z0.2_L45_constant_density/CI609sm.html new file mode 100644 index 00000000..85defec3 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CI609sm.png b/models/smc_Z0.2_L45_constant_density/CI609sm.png new file mode 100644 index 00000000..e285c1ee Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CI609sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.fits new file mode 100644 index 00000000..b381931e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.html b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.html new file mode 100644 index 00000000..e0a8928e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.png b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.png new file mode 100644 index 00000000..8e00daea Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_13CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.fits new file mode 100644 index 00000000..171320e6 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.html b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.html new file mode 100644 index 00000000..0f15630b --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.png b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.png new file mode 100644 index 00000000..7c692bc0 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_13CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.fits new file mode 100644 index 00000000..b4358c07 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.html b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.html new file mode 100644 index 00000000..bd4e19de --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.png b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.png new file mode 100644 index 00000000..6dbd3779 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CI609sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.fits new file mode 100644 index 00000000..84cdcc21 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.html new file mode 100644 index 00000000..e70c5a4d --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.png new file mode 100644 index 00000000..da18e708 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.fits new file mode 100644 index 00000000..4f99e000 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.html b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.html new file mode 100644 index 00000000..fa8833e5 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.png b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.png new file mode 100644 index 00000000..d1fc13cf Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.fits new file mode 100644 index 00000000..47d7a1cb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.html b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.html new file mode 100644 index 00000000..af217dcc --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.png b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.png new file mode 100644 index 00000000..66ca3db0 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO32sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.fits new file mode 100644 index 00000000..1537a0e2 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.html new file mode 100644 index 00000000..ff88c166 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.png new file mode 100644 index 00000000..01fc7d3f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.fits b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.fits new file mode 100644 index 00000000..b6237020 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.html b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.html new file mode 100644 index 00000000..12072b89 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / I<sub>FIR</sub> Intensity Ratio + +
+

+[C II] 158 µm / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.png b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.png new file mode 100644 index 00000000..10c99ecd Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.fits b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.fits new file mode 100644 index 00000000..8ecf011b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.html b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.html new file mode 100644 index 00000000..b06c0015 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [O I] 145 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [O I] 145 µm Intensity Ratio + +
+

+[C II] 158 µm / [O I] 145 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.png b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.png new file mode 100644 index 00000000..91c12126 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158_OI145sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158sm.fits b/models/smc_Z0.2_L45_constant_density/CII158sm.fits new file mode 100644 index 00000000..9ed6ae0a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CII158sm.html b/models/smc_Z0.2_L45_constant_density/CII158sm.html new file mode 100644 index 00000000..f1cf1407 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CII158sm.png b/models/smc_Z0.2_L45_constant_density/CII158sm.png new file mode 100644 index 00000000..c04775cc Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CII158sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.fits new file mode 100644 index 00000000..71c913d6 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.html new file mode 100644 index 00000000..bb8dd25c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.png new file mode 100644 index 00000000..4a82762c Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.fits new file mode 100644 index 00000000..270c1733 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.html new file mode 100644 index 00000000..54e80002 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.png new file mode 100644 index 00000000..af2efe61 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.fits b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.fits new file mode 100644 index 00000000..7572513f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.html b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.html new file mode 100644 index 00000000..664ac050 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.png b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.png new file mode 100644 index 00000000..71810c0b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO109_CO76sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CO10sm.fits new file mode 100644 index 00000000..f4062495 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO10sm.html b/models/smc_Z0.2_L45_constant_density/CO10sm.html new file mode 100644 index 00000000..0a3d5f9f --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO10sm.png b/models/smc_Z0.2_L45_constant_density/CO10sm.png new file mode 100644 index 00000000..02aaf482 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.fits new file mode 100644 index 00000000..df93a96e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.html new file mode 100644 index 00000000..b4d1524e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.png new file mode 100644 index 00000000..ab272908 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.fits new file mode 100644 index 00000000..a79ccac1 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.html new file mode 100644 index 00000000..4b61ebd4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.png new file mode 100644 index 00000000..6a52deb7 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.fits b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.fits new file mode 100644 index 00000000..173cde45 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.html b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.html new file mode 100644 index 00000000..f65fc70c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=8-7) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=8-7) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=8-7) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.png b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.png new file mode 100644 index 00000000..fb46944e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110_CO87sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110sm.fits b/models/smc_Z0.2_L45_constant_density/CO1110sm.fits new file mode 100644 index 00000000..ae5b3897 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1110sm.html b/models/smc_Z0.2_L45_constant_density/CO1110sm.html new file mode 100644 index 00000000..43157dc2 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1110sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1110sm.png b/models/smc_Z0.2_L45_constant_density/CO1110sm.png new file mode 100644 index 00000000..933480db Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1110sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.fits new file mode 100644 index 00000000..7e361de1 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.html new file mode 100644 index 00000000..ba3a2436 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.png new file mode 100644 index 00000000..d78dcc39 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1211_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.fits new file mode 100644 index 00000000..90e4bddd Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.html new file mode 100644 index 00000000..357089e2 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.png new file mode 100644 index 00000000..5772a50d Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1211_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.fits new file mode 100644 index 00000000..7cb6fbed Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.html new file mode 100644 index 00000000..56ffd0de --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.png new file mode 100644 index 00000000..67e40289 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1312_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.fits new file mode 100644 index 00000000..3b5dd653 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.html new file mode 100644 index 00000000..83c37729 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.png new file mode 100644 index 00000000..cf33b62c Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1312_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.fits new file mode 100644 index 00000000..4424d661 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.html new file mode 100644 index 00000000..c53ff5b4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.png new file mode 100644 index 00000000..ca9dbc76 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1413_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.fits new file mode 100644 index 00000000..8ee1a967 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.html new file mode 100644 index 00000000..b575c971 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.png new file mode 100644 index 00000000..f07bd8ca Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1413_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.fits new file mode 100644 index 00000000..80a8874f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.html new file mode 100644 index 00000000..7cc19bda --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.png new file mode 100644 index 00000000..2db068a6 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1514_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.fits new file mode 100644 index 00000000..92538b83 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.html new file mode 100644 index 00000000..c9018dca --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.png new file mode 100644 index 00000000..eaba270f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1514_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.fits new file mode 100644 index 00000000..0bb83553 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.html new file mode 100644 index 00000000..b64f3d14 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.png new file mode 100644 index 00000000..5904d771 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1615_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.fits new file mode 100644 index 00000000..be807f49 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.html new file mode 100644 index 00000000..aec4ba3e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.png new file mode 100644 index 00000000..3eb8d3b1 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1615_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.fits new file mode 100644 index 00000000..28412289 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.html new file mode 100644 index 00000000..d2bf1cae --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.png new file mode 100644 index 00000000..e5b9d692 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1716_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.fits new file mode 100644 index 00000000..ebcba07f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.html new file mode 100644 index 00000000..bbf4b3bb --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.png new file mode 100644 index 00000000..5847756a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1716_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.fits new file mode 100644 index 00000000..20a06e0f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.html new file mode 100644 index 00000000..a8b1882e --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.png new file mode 100644 index 00000000..08978f3a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1817_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.fits new file mode 100644 index 00000000..66438302 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.html new file mode 100644 index 00000000..8e2000de --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.png new file mode 100644 index 00000000..a910e1c9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO1817_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.fits new file mode 100644 index 00000000..91b8ef94 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.html new file mode 100644 index 00000000..4531b95c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.png new file mode 100644 index 00000000..554aee0e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO21_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CO21sm.fits new file mode 100644 index 00000000..607c9889 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO21sm.html b/models/smc_Z0.2_L45_constant_density/CO21sm.html new file mode 100644 index 00000000..2cc36520 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO21sm.png b/models/smc_Z0.2_L45_constant_density/CO21sm.png new file mode 100644 index 00000000..8b2715fa Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.fits new file mode 100644 index 00000000..dc731e04 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.html new file mode 100644 index 00000000..6c882baf --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.png new file mode 100644 index 00000000..42ca140c Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.fits new file mode 100644 index 00000000..76dcd2cf Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.html b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.html new file mode 100644 index 00000000..6dd908af --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.png b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.png new file mode 100644 index 00000000..75ab27e9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32sm.fits b/models/smc_Z0.2_L45_constant_density/CO32sm.fits new file mode 100644 index 00000000..0431a22e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO32sm.html b/models/smc_Z0.2_L45_constant_density/CO32sm.html new file mode 100644 index 00000000..b51c6842 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO32sm.png b/models/smc_Z0.2_L45_constant_density/CO32sm.png new file mode 100644 index 00000000..90f0ae79 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO32sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.fits new file mode 100644 index 00000000..61ac8586 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.html b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.html new file mode 100644 index 00000000..05247928 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.png b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.png new file mode 100644 index 00000000..21848833 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO43sm.fits b/models/smc_Z0.2_L45_constant_density/CO43sm.fits new file mode 100644 index 00000000..906186ff Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO43sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO43sm.html b/models/smc_Z0.2_L45_constant_density/CO43sm.html new file mode 100644 index 00000000..f3cda7e4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO43sm.png b/models/smc_Z0.2_L45_constant_density/CO43sm.png new file mode 100644 index 00000000..80931cac Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO43sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO54sm.fits new file mode 100644 index 00000000..66b11def Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO54sm.html new file mode 100644 index 00000000..17144359 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO54sm.png new file mode 100644 index 00000000..724ef45b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.fits new file mode 100644 index 00000000..1e84a0a3 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.html new file mode 100644 index 00000000..727acbd5 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.png new file mode 100644 index 00000000..3314d29b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO65_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO65sm.fits new file mode 100644 index 00000000..8a757050 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO65sm.html new file mode 100644 index 00000000..a1bf67e3 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO65sm.png new file mode 100644 index 00000000..b4c212be Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.fits b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.fits new file mode 100644 index 00000000..8678f565 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.html b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.html new file mode 100644 index 00000000..6e377495 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.png b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.png new file mode 100644 index 00000000..9d60e68b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO10sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.fits b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.fits new file mode 100644 index 00000000..7536af15 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.html b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.html new file mode 100644 index 00000000..8a02b912 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.png b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.png new file mode 100644 index 00000000..ce82631d Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.fits b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.fits new file mode 100644 index 00000000..0b3de4bf Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.html b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.html new file mode 100644 index 00000000..98182fc0 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.png b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.png new file mode 100644 index 00000000..32942b79 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO43sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.fits new file mode 100644 index 00000000..4abc3551 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.html new file mode 100644 index 00000000..e4aca992 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.png new file mode 100644 index 00000000..e92d9bb7 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.fits new file mode 100644 index 00000000..9391e8c1 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.html new file mode 100644 index 00000000..21be518c --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.png new file mode 100644 index 00000000..47f50882 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76sm.fits b/models/smc_Z0.2_L45_constant_density/CO76sm.fits new file mode 100644 index 00000000..504d0bdb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO76sm.html b/models/smc_Z0.2_L45_constant_density/CO76sm.html new file mode 100644 index 00000000..607c4218 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO76sm.png b/models/smc_Z0.2_L45_constant_density/CO76sm.png new file mode 100644 index 00000000..713cec4b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO76sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.fits new file mode 100644 index 00000000..0bd4b894 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.html new file mode 100644 index 00000000..1da9c484 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.png new file mode 100644 index 00000000..35e8f0de Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.fits new file mode 100644 index 00000000..a1fb5523 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.html new file mode 100644 index 00000000..b4240dc0 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.png new file mode 100644 index 00000000..5f3455f9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87sm.fits b/models/smc_Z0.2_L45_constant_density/CO87sm.fits new file mode 100644 index 00000000..e061b87e Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO87sm.html b/models/smc_Z0.2_L45_constant_density/CO87sm.html new file mode 100644 index 00000000..6d08326b --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO87sm.png b/models/smc_Z0.2_L45_constant_density/CO87sm.png new file mode 100644 index 00000000..ce7ec9a8 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO87sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.fits b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.fits new file mode 100644 index 00000000..432977aa Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.html b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.html new file mode 100644 index 00000000..e0b5b461 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.png b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.png new file mode 100644 index 00000000..cf6df3c4 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO98_CO54sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.fits b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.fits new file mode 100644 index 00000000..5cb9c6b0 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.html b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.html new file mode 100644 index 00000000..04f4ff31 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.png b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.png new file mode 100644 index 00000000..7db4b5a6 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/CO98_CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S0sm.fits b/models/smc_Z0.2_L45_constant_density/H200S0sm.fits new file mode 100644 index 00000000..98970f5a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S0sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S0sm.html b/models/smc_Z0.2_L45_constant_density/H200S0sm.html new file mode 100644 index 00000000..640465a4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(0) 28.2 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(0) 28.2 µm Intensity + +
+

+H20-0S(0) 28.2 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S0sm.png b/models/smc_Z0.2_L45_constant_density/H200S0sm.png new file mode 100644 index 00000000..a96f3299 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S0sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S1sm.fits b/models/smc_Z0.2_L45_constant_density/H200S1sm.fits new file mode 100644 index 00000000..d0f60da5 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S1sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S1sm.html b/models/smc_Z0.2_L45_constant_density/H200S1sm.html new file mode 100644 index 00000000..97fffa7f --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(1) 17 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(1) 17 µm Intensity + +
+

+H20-0S(1) 17 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S1sm.png b/models/smc_Z0.2_L45_constant_density/H200S1sm.png new file mode 100644 index 00000000..0af1f07b Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S1sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.fits b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.fits new file mode 100644 index 00000000..48d8b375 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.html b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.html new file mode 100644 index 00000000..23cd365f --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.png b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.png new file mode 100644 index 00000000..820c6923 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2_H200S0sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.fits b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.fits new file mode 100644 index 00000000..8730be2f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.html b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.html new file mode 100644 index 00000000..0dfb74de --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.png b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.png new file mode 100644 index 00000000..06b72667 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2_H200S1sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2sm.fits b/models/smc_Z0.2_L45_constant_density/H200S2sm.fits new file mode 100644 index 00000000..a2d728a0 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S2sm.html b/models/smc_Z0.2_L45_constant_density/H200S2sm.html new file mode 100644 index 00000000..8e278dbd --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm Intensity + +
+

+H20-0S(2) 12.3 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S2sm.png b/models/smc_Z0.2_L45_constant_density/H200S2sm.png new file mode 100644 index 00000000..eb52d3d3 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S2sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.fits b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.fits new file mode 100644 index 00000000..eba84890 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.html b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.html new file mode 100644 index 00000000..229d8d1f --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.png b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.png new file mode 100644 index 00000000..69aec506 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S0sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.fits b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.fits new file mode 100644 index 00000000..3d0e2af2 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.html b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.html new file mode 100644 index 00000000..3acb2a0a --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.png b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.png new file mode 100644 index 00000000..7e9f7ab9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S1sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.fits b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.fits new file mode 100644 index 00000000..684b3d5f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.html b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.html new file mode 100644 index 00000000..454ab657 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(2) 12.3 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.png b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.png new file mode 100644 index 00000000..57137ee8 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3_H200S2sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3sm.fits b/models/smc_Z0.2_L45_constant_density/H200S3sm.fits new file mode 100644 index 00000000..ef6ea778 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H200S3sm.html b/models/smc_Z0.2_L45_constant_density/H200S3sm.html new file mode 100644 index 00000000..7dbacefa --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H200S3sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm Intensity + +
+

+H20-0S(3) 9.7 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H200S3sm.png b/models/smc_Z0.2_L45_constant_density/H200S3sm.png new file mode 100644 index 00000000..63d26cfa Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H200S3sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.fits b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.fits new file mode 100644 index 00000000..841b79ca Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.html b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.html new file mode 100644 index 00000000..fbaa3e25 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>2-1S(1) 2.24 µm / H<sub>2</sub>1-0S(1) 2.12 µm Intensity Ratio + +
+

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.png b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.png new file mode 100644 index 00000000..b5df6bb9 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/H221S1_H210S1sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.fits b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.fits new file mode 100644 index 00000000..d07152f6 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.html b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.html new file mode 100644 index 00000000..9f53b386 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 145 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.png b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.png new file mode 100644 index 00000000..540db9eb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.fits b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.fits new file mode 100644 index 00000000..ab966303 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.html b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.html new file mode 100644 index 00000000..1427aae4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.png b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.png new file mode 100644 index 00000000..e4b30580 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145_13CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.fits b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.fits new file mode 100644 index 00000000..f7baab05 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.html b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.html new file mode 100644 index 00000000..0734bea5 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / [O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / [O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm / [O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.png b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.png new file mode 100644 index 00000000..5b462f82 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145_OI63sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145sm.fits b/models/smc_Z0.2_L45_constant_density/OI145sm.fits new file mode 100644 index 00000000..0dc8111f Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI145sm.html b/models/smc_Z0.2_L45_constant_density/OI145sm.html new file mode 100644 index 00000000..625f8a55 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI145sm.png b/models/smc_Z0.2_L45_constant_density/OI145sm.png new file mode 100644 index 00000000..5ca7c344 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI145sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.fits b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.fits new file mode 100644 index 00000000..ce15ca30 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.html b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.html new file mode 100644 index 00000000..224e3a01 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.png b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.png new file mode 100644 index 00000000..a4b06326 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.fits b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.fits new file mode 100644 index 00000000..c17ce648 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.html b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.html new file mode 100644 index 00000000..941ada0d --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.png b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.png new file mode 100644 index 00000000..69f517f4 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63_13CO65sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.fits b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.fits new file mode 100644 index 00000000..98596c7a Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.html b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.html new file mode 100644 index 00000000..f06e2ce2 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / [C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / [C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.png b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.png new file mode 100644 index 00000000..8ba1deea Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63_CII158sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63sm.fits b/models/smc_Z0.2_L45_constant_density/OI63sm.fits new file mode 100644 index 00000000..fcee3bfb Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/OI63sm.html b/models/smc_Z0.2_L45_constant_density/OI63sm.html new file mode 100644 index 00000000..241dbce4 --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/OI63sm.png b/models/smc_Z0.2_L45_constant_density/OI63sm.png new file mode 100644 index 00000000..5355f751 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/OI63sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.fits b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.fits new file mode 100644 index 00000000..e8e9e3c4 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.fits differ diff --git a/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.html b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.html new file mode 100644 index 00000000..d7f3840d --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+Temperature at AV = 0.01 +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + Temperature at A<sub>V</sub> = 0.01 + +
+

+Temperature at AV = 0.01 emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=45 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.png b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.png new file mode 100644 index 00000000..a44a6722 Binary files /dev/null and b/models/smc_Z0.2_L45_constant_density/TSAV0p01sm.png differ diff --git a/models/smc_Z0.2_L45_constant_density/index.html b/models/smc_Z0.2_L45_constant_density/index.html new file mode 100644 index 00000000..ef275fbc --- /dev/null +++ b/models/smc_Z0.2_L45_constant_density/index.html @@ -0,0 +1,73 @@ + + + + + + + + + +
+
+ +

+Wolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=45

+

+Below are links to the individual FITS files +and plots in the smc z=0.2 losangle=45 ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. + + + + + + + + + + + + + + + + + + + + + + + + + +
[O I] 63 µm / [C II] 158 µm Intensity Ratio[O I] 63 µm / 13CO(J=6-5) Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio
[O I] 145 µm / [O I] 63 µm Intensity Ratio[O I] 145 µm / 13CO(J=6-5) Intensity Ratio[C I] 370 µm / [C I] 609 µm Intensity Ratio[C II] 158 µm / [C I] 609 µm Intensity Ratio
[C II] 158 µm / [O I] 145 µm Intensity Ratio[C II] 158 µm / IFIR Intensity Ratio[C II] 158 µm / CO(J=1-0) Intensity Ratio[C II] 158 µm / CO(J=2-1) Intensity Ratio
[C II] 158 µm / CO(J=3-2) Intensity Ratio[C II] 158 µm / CO(J=6-5) Intensity Ratio[C II] 158 µm / 13CO(J=1-0) Intensity Ratio[C II] 158 µm / 13CO(J=6-5) Intensity Ratio
CO(J=2-1) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=4-3) Intensity Ratio
[C I] 609 µm / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=2-1) Intensity Ratio
[C I] 609 µm / 13CO(J=3-2) Intensity RatioCO(J=4-3) / CO(J=2-1) Intensity RatioCO(J=6-5) / CO(J=1-0) Intensity RatioCO(J=7-6) / CO(J=1-0) Intensity Ratio
CO(J=7-6) / CO(J=2-1) Intensity RatioCO(J=7-6) / CO(J=4-3) Intensity RatioCO(J=7-6) / CO(J=5-4) Intensity RatioCO(J=7-6) / CO(J=6-5) Intensity Ratio
CO(J=8-7) / CO(J=5-4) Intensity RatioCO(J=8-7) / CO(J=6-5) Intensity RatioCO(J=9-8) / CO(J=5-4) Intensity RatioCO(J=9-8) / CO(J=6-5) Intensity Ratio
CO(J=10-9) / CO(J=5-4) Intensity RatioCO(J=10-9) / CO(J=6-5) Intensity RatioCO(J=10-9) / CO(J=7-6) Intensity RatioCO(J=11-10) / CO(J=5-4) Intensity Ratio
CO(J=11-10) / CO(J=6-5) Intensity RatioCO(J=11-10) / CO(J=8-7) Intensity RatioCO(J=12-11) / CO(J=5-4) Intensity RatioCO(J=12-11) / CO(J=6-5) Intensity Ratio
CO(J=13-12) / CO(J=5-4) Intensity RatioCO(J=13-12) / CO(J=6-5) Intensity RatioCO(J=14-13) / CO(J=5-4) Intensity RatioCO(J=14-13) / CO(J=6-5) Intensity Ratio
CO(J=15-14) / CO(J=5-4) Intensity RatioCO(J=15-14) / CO(J=6-5) Intensity RatioCO(J=16-15) / CO(J=5-4) Intensity RatioCO(J=16-15) / CO(J=6-5) Intensity Ratio
CO(J=17-16) / CO(J=5-4) Intensity RatioCO(J=17-16) / CO(J=6-5) Intensity RatioCO(J=18-17) / CO(J=5-4) Intensity RatioCO(J=18-17) / CO(J=6-5) Intensity Ratio
13CO(J=1-0) / CO(J=1-0) Intensity Ratio13CO(J=2-1) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / CO(J=2-1) Intensity Ratio13CO(J=4-3) / CO(J=2-1) Intensity Ratio
13CO(J=5-4) / CO(J=2-1) Intensity Ratio13CO(J=6-5) / CO(J=2-1) Intensity Ratio13CO(J=7-6) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio
H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio
H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity RatioH22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio[C I] 370 µm Intensity[C I] 609 µm Intensity
[C II] 158 µm Intensity[O I] 63 µm Intensity[O I] 145 µm IntensityCO(J=1-0) Intensity
CO(J=2-1) IntensityCO(J=3-2) IntensityCO(J=4-3) IntensityCO(J=5-4) Intensity
CO(J=6-5) IntensityCO(J=7-6) IntensityCO(J=8-7) IntensityCO(J=11-10) Intensity
13CO(J=1-0) Intensity13CO(J=2-1) Intensity13CO(J=3-2) IntensityH20-0S(3) 9.7 µm Intensity
H20-0S(2) 12.3 µm IntensityH20-0S(1) 17 µm IntensityH20-0S(0) 28.2 µm IntensityTemperature at AV = 0.01
+

+
+
+ + + + diff --git a/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.fits new file mode 100644 index 00000000..08de2cf7 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.html b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.html new file mode 100644 index 00000000..fe34828e --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) / CO(J=1-0) Intensity Ratio + +
+

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.png b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.png new file mode 100644 index 00000000..9f198c64 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO10_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO10sm.fits b/models/smc_Z0.2_L60_constant_density/13CO10sm.fits new file mode 100644 index 00000000..80e89c58 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO10sm.html b/models/smc_Z0.2_L60_constant_density/13CO10sm.html new file mode 100644 index 00000000..8a49c22b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) Intensity + +
+

+13CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO10sm.png b/models/smc_Z0.2_L60_constant_density/13CO10sm.png new file mode 100644 index 00000000..e046c551 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.fits new file mode 100644 index 00000000..cf02fa9f Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.html new file mode 100644 index 00000000..835b7a3f --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.png new file mode 100644 index 00000000..afa45cdf Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO21_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO21sm.fits new file mode 100644 index 00000000..2c202086 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO21sm.html new file mode 100644 index 00000000..e4598188 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) Intensity + +
+

+13CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO21sm.png new file mode 100644 index 00000000..bef6cfc4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.fits b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.fits new file mode 100644 index 00000000..bf9505aa Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.html b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.html new file mode 100644 index 00000000..82156e4d --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.png b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.png new file mode 100644 index 00000000..8d2cd659 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32_13CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.fits new file mode 100644 index 00000000..79d93106 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.html new file mode 100644 index 00000000..b7cddab7 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.png new file mode 100644 index 00000000..80b2c69e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32sm.fits b/models/smc_Z0.2_L60_constant_density/13CO32sm.fits new file mode 100644 index 00000000..c2302138 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO32sm.html b/models/smc_Z0.2_L60_constant_density/13CO32sm.html new file mode 100644 index 00000000..5bacd415 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) Intensity + +
+

+13CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO32sm.png b/models/smc_Z0.2_L60_constant_density/13CO32sm.png new file mode 100644 index 00000000..c1f93afd Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO32sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.fits new file mode 100644 index 00000000..7a2af685 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.html new file mode 100644 index 00000000..bec63c32 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.png new file mode 100644 index 00000000..3fc00a43 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.fits new file mode 100644 index 00000000..954f0046 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.html new file mode 100644 index 00000000..8c74a262 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=5-4) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.png new file mode 100644 index 00000000..f88b5df0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO54_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.fits new file mode 100644 index 00000000..f7db160c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.html new file mode 100644 index 00000000..ec37417a --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=6-5) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.png new file mode 100644 index 00000000..c3f92b07 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO65_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.fits new file mode 100644 index 00000000..66050f77 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.html b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.html new file mode 100644 index 00000000..3cbfc8b7 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.png b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.png new file mode 100644 index 00000000..b9ec9b33 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/13CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.fits b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.fits new file mode 100644 index 00000000..2dae82d8 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.html b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.html new file mode 100644 index 00000000..e79aea41 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm / [C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.png b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.png new file mode 100644 index 00000000..da4b81ec Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI370_CI609sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI370sm.fits b/models/smc_Z0.2_L60_constant_density/CI370sm.fits new file mode 100644 index 00000000..933720aa Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI370sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI370sm.html b/models/smc_Z0.2_L60_constant_density/CI370sm.html new file mode 100644 index 00000000..6edccb79 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI370sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI370sm.png b/models/smc_Z0.2_L60_constant_density/CI370sm.png new file mode 100644 index 00000000..146f7e64 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI370sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.fits new file mode 100644 index 00000000..47b3923c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.html b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.html new file mode 100644 index 00000000..6a06186e --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.png b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.png new file mode 100644 index 00000000..1b60d0bf Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.fits new file mode 100644 index 00000000..3e57bdb6 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.html b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.html new file mode 100644 index 00000000..4575cc68 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.png b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.png new file mode 100644 index 00000000..6dbbc95b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.fits new file mode 100644 index 00000000..34f4303c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.html b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.html new file mode 100644 index 00000000..0973b80b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=3-2) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.png b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.png new file mode 100644 index 00000000..829e2e79 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_13CO32sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.fits new file mode 100644 index 00000000..6e606127 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.html new file mode 100644 index 00000000..ae344015 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.png new file mode 100644 index 00000000..2d697e4c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.fits new file mode 100644 index 00000000..d0ea81db Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.html b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.html new file mode 100644 index 00000000..32f4a8c8 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.png b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.png new file mode 100644 index 00000000..b314fc36 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.fits b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.fits new file mode 100644 index 00000000..9d3e9144 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.html b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.html new file mode 100644 index 00000000..e7fa47c4 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=4-3) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.png b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.png new file mode 100644 index 00000000..4a0e593b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609_CO43sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609sm.fits b/models/smc_Z0.2_L60_constant_density/CI609sm.fits new file mode 100644 index 00000000..7b6589dc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CI609sm.html b/models/smc_Z0.2_L60_constant_density/CI609sm.html new file mode 100644 index 00000000..5886779e --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CI609sm.png b/models/smc_Z0.2_L60_constant_density/CI609sm.png new file mode 100644 index 00000000..6c0d3537 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CI609sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.fits new file mode 100644 index 00000000..07e41a63 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.html b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.html new file mode 100644 index 00000000..d7baf9fc --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.png b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.png new file mode 100644 index 00000000..5b75ecf6 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_13CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.fits new file mode 100644 index 00000000..39d3eedc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.html b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.html new file mode 100644 index 00000000..539892af --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.png b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.png new file mode 100644 index 00000000..8543f6a0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_13CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.fits new file mode 100644 index 00000000..4e423248 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.html b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.html new file mode 100644 index 00000000..eac1612e --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.png b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.png new file mode 100644 index 00000000..4e763b38 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CI609sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.fits new file mode 100644 index 00000000..17fe469e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.html new file mode 100644 index 00000000..82852328 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.png new file mode 100644 index 00000000..d18747e3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.fits new file mode 100644 index 00000000..5eda9929 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.html b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.html new file mode 100644 index 00000000..1ef21ac6 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.png b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.png new file mode 100644 index 00000000..d2ee7b97 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.fits new file mode 100644 index 00000000..b53e8bd8 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.html b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.html new file mode 100644 index 00000000..5a2cdd1d --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.png b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.png new file mode 100644 index 00000000..aac797e3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO32sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.fits new file mode 100644 index 00000000..80034650 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.html new file mode 100644 index 00000000..69964054 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.png new file mode 100644 index 00000000..5fb1b844 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.fits b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.fits new file mode 100644 index 00000000..d0effea6 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.html b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.html new file mode 100644 index 00000000..2077f5b3 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / I<sub>FIR</sub> Intensity Ratio + +
+

+[C II] 158 µm / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.png b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.png new file mode 100644 index 00000000..11fe986e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.fits b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.fits new file mode 100644 index 00000000..0f7d0a82 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.html b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.html new file mode 100644 index 00000000..ad1fe83b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [O I] 145 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [O I] 145 µm Intensity Ratio + +
+

+[C II] 158 µm / [O I] 145 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.png b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.png new file mode 100644 index 00000000..9de77a74 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158_OI145sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158sm.fits b/models/smc_Z0.2_L60_constant_density/CII158sm.fits new file mode 100644 index 00000000..c9351bfa Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CII158sm.html b/models/smc_Z0.2_L60_constant_density/CII158sm.html new file mode 100644 index 00000000..c1c8bd81 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CII158sm.png b/models/smc_Z0.2_L60_constant_density/CII158sm.png new file mode 100644 index 00000000..84a90c02 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CII158sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.fits new file mode 100644 index 00000000..994891b9 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.html new file mode 100644 index 00000000..99836b14 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.png new file mode 100644 index 00000000..ef84ce04 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.fits new file mode 100644 index 00000000..3ec5f8b3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.html new file mode 100644 index 00000000..1b32db04 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.png new file mode 100644 index 00000000..b98ec5c4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.fits b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.fits new file mode 100644 index 00000000..38326940 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.html b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.html new file mode 100644 index 00000000..a7bf07cd --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.png b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.png new file mode 100644 index 00000000..221adfea Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO109_CO76sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CO10sm.fits new file mode 100644 index 00000000..f54bbe85 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO10sm.html b/models/smc_Z0.2_L60_constant_density/CO10sm.html new file mode 100644 index 00000000..acf65292 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO10sm.png b/models/smc_Z0.2_L60_constant_density/CO10sm.png new file mode 100644 index 00000000..cd76edf5 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.fits new file mode 100644 index 00000000..537d3dff Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.html new file mode 100644 index 00000000..fe7fe1f3 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.png new file mode 100644 index 00000000..cb935285 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.fits new file mode 100644 index 00000000..20654afc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.html new file mode 100644 index 00000000..5a196a59 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.png new file mode 100644 index 00000000..c08ccc7d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.fits b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.fits new file mode 100644 index 00000000..17a33bff Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.html b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.html new file mode 100644 index 00000000..c64fcea7 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=8-7) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=8-7) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=8-7) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.png b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.png new file mode 100644 index 00000000..414095db Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110_CO87sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110sm.fits b/models/smc_Z0.2_L60_constant_density/CO1110sm.fits new file mode 100644 index 00000000..ab9ab0cc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1110sm.html b/models/smc_Z0.2_L60_constant_density/CO1110sm.html new file mode 100644 index 00000000..d3f17179 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1110sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1110sm.png b/models/smc_Z0.2_L60_constant_density/CO1110sm.png new file mode 100644 index 00000000..0989f825 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1110sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.fits new file mode 100644 index 00000000..ddd610ad Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.html new file mode 100644 index 00000000..9ecd32e4 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.png new file mode 100644 index 00000000..4cb40f2b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1211_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.fits new file mode 100644 index 00000000..047c7ff1 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.html new file mode 100644 index 00000000..66371975 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.png new file mode 100644 index 00000000..f2b6ea84 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1211_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.fits new file mode 100644 index 00000000..e1600b4c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.html new file mode 100644 index 00000000..628b3cd7 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.png new file mode 100644 index 00000000..6fc1f9c9 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1312_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.fits new file mode 100644 index 00000000..64f7d1ea Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.html new file mode 100644 index 00000000..a894f267 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.png new file mode 100644 index 00000000..2d4fe529 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1312_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.fits new file mode 100644 index 00000000..c7f131b4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.html new file mode 100644 index 00000000..32877788 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.png new file mode 100644 index 00000000..fee553dc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1413_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.fits new file mode 100644 index 00000000..25c437a3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.html new file mode 100644 index 00000000..ab93dabe --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.png new file mode 100644 index 00000000..49ee45bb Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1413_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.fits new file mode 100644 index 00000000..5b4f0e75 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.html new file mode 100644 index 00000000..dcb6eb76 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.png new file mode 100644 index 00000000..5b669f66 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1514_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.fits new file mode 100644 index 00000000..7a6e0716 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.html new file mode 100644 index 00000000..6a63d37c --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.png new file mode 100644 index 00000000..3a7b1bb3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1514_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.fits new file mode 100644 index 00000000..6ace69ed Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.html new file mode 100644 index 00000000..5bd3a56f --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.png new file mode 100644 index 00000000..41e258ab Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1615_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.fits new file mode 100644 index 00000000..c59600af Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.html new file mode 100644 index 00000000..cb67ec88 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.png new file mode 100644 index 00000000..1c5f234e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1615_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.fits new file mode 100644 index 00000000..dab72171 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.html new file mode 100644 index 00000000..be966f2e --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.png new file mode 100644 index 00000000..2581be4a Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1716_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.fits new file mode 100644 index 00000000..fe6e784e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.html new file mode 100644 index 00000000..ee632902 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.png new file mode 100644 index 00000000..0f00892b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1716_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.fits new file mode 100644 index 00000000..4ecc31b9 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.html new file mode 100644 index 00000000..26423260 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.png new file mode 100644 index 00000000..19756dfe Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1817_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.fits new file mode 100644 index 00000000..15e8f523 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.html new file mode 100644 index 00000000..446d1f79 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.png new file mode 100644 index 00000000..e69157c4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO1817_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.fits new file mode 100644 index 00000000..49b954f0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.html new file mode 100644 index 00000000..99935d03 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.png new file mode 100644 index 00000000..6a7eb12b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO21_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CO21sm.fits new file mode 100644 index 00000000..f1a6b7dd Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO21sm.html b/models/smc_Z0.2_L60_constant_density/CO21sm.html new file mode 100644 index 00000000..95c980e7 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO21sm.png b/models/smc_Z0.2_L60_constant_density/CO21sm.png new file mode 100644 index 00000000..940e922d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.fits new file mode 100644 index 00000000..6c9aaac1 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.html new file mode 100644 index 00000000..5e1ce90f --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.png new file mode 100644 index 00000000..3f86f382 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.fits new file mode 100644 index 00000000..cbb505ec Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.html b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.html new file mode 100644 index 00000000..b7d70fe9 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.png b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.png new file mode 100644 index 00000000..d9abeb0c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32sm.fits b/models/smc_Z0.2_L60_constant_density/CO32sm.fits new file mode 100644 index 00000000..50b3d5c0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO32sm.html b/models/smc_Z0.2_L60_constant_density/CO32sm.html new file mode 100644 index 00000000..f93c5549 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO32sm.png b/models/smc_Z0.2_L60_constant_density/CO32sm.png new file mode 100644 index 00000000..4e5423d3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO32sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.fits new file mode 100644 index 00000000..95885502 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.html b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.html new file mode 100644 index 00000000..b0517361 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.png b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.png new file mode 100644 index 00000000..f79105bb Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO43sm.fits b/models/smc_Z0.2_L60_constant_density/CO43sm.fits new file mode 100644 index 00000000..2f9fee0d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO43sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO43sm.html b/models/smc_Z0.2_L60_constant_density/CO43sm.html new file mode 100644 index 00000000..d513cddd --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO43sm.png b/models/smc_Z0.2_L60_constant_density/CO43sm.png new file mode 100644 index 00000000..f7f27465 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO43sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO54sm.fits new file mode 100644 index 00000000..30e4e2a5 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO54sm.html new file mode 100644 index 00000000..de4d8768 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO54sm.png new file mode 100644 index 00000000..7c92be1d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.fits new file mode 100644 index 00000000..0ba67858 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.html new file mode 100644 index 00000000..061d765b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.png new file mode 100644 index 00000000..320048f1 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO65_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO65sm.fits new file mode 100644 index 00000000..32629928 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO65sm.html new file mode 100644 index 00000000..0a290e4b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO65sm.png new file mode 100644 index 00000000..8357d951 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.fits b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.fits new file mode 100644 index 00000000..5d2a26fa Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.html b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.html new file mode 100644 index 00000000..742bea04 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.png b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.png new file mode 100644 index 00000000..c241986c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO10sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.fits b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.fits new file mode 100644 index 00000000..33988de5 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.html b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.html new file mode 100644 index 00000000..7966ff2c --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.png b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.png new file mode 100644 index 00000000..2a884e0c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.fits b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.fits new file mode 100644 index 00000000..dcf039f4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.html b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.html new file mode 100644 index 00000000..ea362612 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.png b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.png new file mode 100644 index 00000000..eb9ca218 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO43sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.fits new file mode 100644 index 00000000..f89cd5d2 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.html new file mode 100644 index 00000000..8cb53923 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.png new file mode 100644 index 00000000..a3c2fca0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.fits new file mode 100644 index 00000000..d5f4e435 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.html new file mode 100644 index 00000000..fa3fdf8b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.png new file mode 100644 index 00000000..6c69e2c5 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76sm.fits b/models/smc_Z0.2_L60_constant_density/CO76sm.fits new file mode 100644 index 00000000..fd70e50d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO76sm.html b/models/smc_Z0.2_L60_constant_density/CO76sm.html new file mode 100644 index 00000000..0dbd1b95 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO76sm.png b/models/smc_Z0.2_L60_constant_density/CO76sm.png new file mode 100644 index 00000000..80ef325f Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO76sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.fits new file mode 100644 index 00000000..2dac18db Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.html new file mode 100644 index 00000000..30d2da93 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.png new file mode 100644 index 00000000..208880d1 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.fits new file mode 100644 index 00000000..03c9a4ab Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.html new file mode 100644 index 00000000..5b1c5c45 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.png new file mode 100644 index 00000000..7071d84d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87sm.fits b/models/smc_Z0.2_L60_constant_density/CO87sm.fits new file mode 100644 index 00000000..c56be775 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO87sm.html b/models/smc_Z0.2_L60_constant_density/CO87sm.html new file mode 100644 index 00000000..f9fae539 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO87sm.png b/models/smc_Z0.2_L60_constant_density/CO87sm.png new file mode 100644 index 00000000..87f8a254 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO87sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.fits b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.fits new file mode 100644 index 00000000..53fc63f8 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.html b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.html new file mode 100644 index 00000000..c5130814 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.png b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.png new file mode 100644 index 00000000..e64a0ab0 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO98_CO54sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.fits b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.fits new file mode 100644 index 00000000..2f095a4c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.html b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.html new file mode 100644 index 00000000..00490500 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.png b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.png new file mode 100644 index 00000000..842e8912 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/CO98_CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S0sm.fits b/models/smc_Z0.2_L60_constant_density/H200S0sm.fits new file mode 100644 index 00000000..08741ecc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S0sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S0sm.html b/models/smc_Z0.2_L60_constant_density/H200S0sm.html new file mode 100644 index 00000000..b87f6647 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(0) 28.2 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(0) 28.2 µm Intensity + +
+

+H20-0S(0) 28.2 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S0sm.png b/models/smc_Z0.2_L60_constant_density/H200S0sm.png new file mode 100644 index 00000000..dc113385 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S0sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S1sm.fits b/models/smc_Z0.2_L60_constant_density/H200S1sm.fits new file mode 100644 index 00000000..c1cbf6de Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S1sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S1sm.html b/models/smc_Z0.2_L60_constant_density/H200S1sm.html new file mode 100644 index 00000000..8bc1cdfb --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(1) 17 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(1) 17 µm Intensity + +
+

+H20-0S(1) 17 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S1sm.png b/models/smc_Z0.2_L60_constant_density/H200S1sm.png new file mode 100644 index 00000000..e9523338 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S1sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.fits b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.fits new file mode 100644 index 00000000..af6910fe Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.html b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.html new file mode 100644 index 00000000..609279c6 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.png b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.png new file mode 100644 index 00000000..0a5156bc Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2_H200S0sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.fits b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.fits new file mode 100644 index 00000000..01965808 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.html b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.html new file mode 100644 index 00000000..68ccb598 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.png b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.png new file mode 100644 index 00000000..49c28ae9 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2_H200S1sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2sm.fits b/models/smc_Z0.2_L60_constant_density/H200S2sm.fits new file mode 100644 index 00000000..06582b3d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S2sm.html b/models/smc_Z0.2_L60_constant_density/H200S2sm.html new file mode 100644 index 00000000..505fcefd --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm Intensity + +
+

+H20-0S(2) 12.3 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S2sm.png b/models/smc_Z0.2_L60_constant_density/H200S2sm.png new file mode 100644 index 00000000..b7748145 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S2sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.fits b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.fits new file mode 100644 index 00000000..45228e07 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.html b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.html new file mode 100644 index 00000000..0331f1f3 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.png b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.png new file mode 100644 index 00000000..8fb4a219 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S0sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.fits b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.fits new file mode 100644 index 00000000..751fbfe3 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.html b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.html new file mode 100644 index 00000000..99db40f5 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.png b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.png new file mode 100644 index 00000000..c307e003 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S1sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.fits b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.fits new file mode 100644 index 00000000..54d4c548 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.html b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.html new file mode 100644 index 00000000..a446135f --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(2) 12.3 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.png b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.png new file mode 100644 index 00000000..62ad3e73 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3_H200S2sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3sm.fits b/models/smc_Z0.2_L60_constant_density/H200S3sm.fits new file mode 100644 index 00000000..501c080e Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H200S3sm.html b/models/smc_Z0.2_L60_constant_density/H200S3sm.html new file mode 100644 index 00000000..c1628e20 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H200S3sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm Intensity + +
+

+H20-0S(3) 9.7 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H200S3sm.png b/models/smc_Z0.2_L60_constant_density/H200S3sm.png new file mode 100644 index 00000000..0ec4211d Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H200S3sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.fits b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.fits new file mode 100644 index 00000000..2cc7a3cf Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.html b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.html new file mode 100644 index 00000000..77586bee --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>2-1S(1) 2.24 µm / H<sub>2</sub>1-0S(1) 2.12 µm Intensity Ratio + +
+

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.png b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.png new file mode 100644 index 00000000..2850a54f Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/H221S1_H210S1sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.fits b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.fits new file mode 100644 index 00000000..b2cbf36c Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.html b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.html new file mode 100644 index 00000000..e9174798 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 145 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.png b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.png new file mode 100644 index 00000000..57ce9926 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.fits b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.fits new file mode 100644 index 00000000..8d393c23 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.html b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.html new file mode 100644 index 00000000..6a767d7b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.png b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.png new file mode 100644 index 00000000..e8c2db43 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145_13CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.fits b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.fits new file mode 100644 index 00000000..c2a03185 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.html b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.html new file mode 100644 index 00000000..e05b57ae --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / [O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / [O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm / [O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.png b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.png new file mode 100644 index 00000000..b86e3a01 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145_OI63sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145sm.fits b/models/smc_Z0.2_L60_constant_density/OI145sm.fits new file mode 100644 index 00000000..c88e2cd7 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI145sm.html b/models/smc_Z0.2_L60_constant_density/OI145sm.html new file mode 100644 index 00000000..03411e6c --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI145sm.png b/models/smc_Z0.2_L60_constant_density/OI145sm.png new file mode 100644 index 00000000..f74f31db Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI145sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.fits b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.fits new file mode 100644 index 00000000..0f2e2bd8 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.html b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.html new file mode 100644 index 00000000..9c7acbdb --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.png b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.png new file mode 100644 index 00000000..154d8182 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.fits b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.fits new file mode 100644 index 00000000..9d2b7afd Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.html b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.html new file mode 100644 index 00000000..aecf760b --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.png b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.png new file mode 100644 index 00000000..29d9c244 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63_13CO65sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.fits b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.fits new file mode 100644 index 00000000..f93ab870 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.html b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.html new file mode 100644 index 00000000..778d3305 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / [C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / [C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.png b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.png new file mode 100644 index 00000000..b3512c50 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63_CII158sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63sm.fits b/models/smc_Z0.2_L60_constant_density/OI63sm.fits new file mode 100644 index 00000000..87ea5a71 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/OI63sm.html b/models/smc_Z0.2_L60_constant_density/OI63sm.html new file mode 100644 index 00000000..cbce4fc3 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/OI63sm.png b/models/smc_Z0.2_L60_constant_density/OI63sm.png new file mode 100644 index 00000000..a9997e9b Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/OI63sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.fits b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.fits new file mode 100644 index 00000000..e8e9e3c4 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.fits differ diff --git a/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.html b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.html new file mode 100644 index 00000000..06106dd1 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+Temperature at AV = 0.01 +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + Temperature at A<sub>V</sub> = 0.01 + +
+

+Temperature at AV = 0.01 emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=60 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.png b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.png new file mode 100644 index 00000000..a44a6722 Binary files /dev/null and b/models/smc_Z0.2_L60_constant_density/TSAV0p01sm.png differ diff --git a/models/smc_Z0.2_L60_constant_density/index.html b/models/smc_Z0.2_L60_constant_density/index.html new file mode 100644 index 00000000..2e2d5359 --- /dev/null +++ b/models/smc_Z0.2_L60_constant_density/index.html @@ -0,0 +1,73 @@ + + + + + + + + + +
+
+ +

+Wolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=60

+

+Below are links to the individual FITS files +and plots in the smc z=0.2 losangle=60 ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. + + + + + + + + + + + + + + + + + + + + + + + + + +
[O I] 63 µm / [C II] 158 µm Intensity Ratio[O I] 63 µm / 13CO(J=6-5) Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio
[O I] 145 µm / [O I] 63 µm Intensity Ratio[O I] 145 µm / 13CO(J=6-5) Intensity Ratio[C I] 370 µm / [C I] 609 µm Intensity Ratio[C II] 158 µm / [C I] 609 µm Intensity Ratio
[C II] 158 µm / [O I] 145 µm Intensity Ratio[C II] 158 µm / IFIR Intensity Ratio[C II] 158 µm / CO(J=1-0) Intensity Ratio[C II] 158 µm / CO(J=2-1) Intensity Ratio
[C II] 158 µm / CO(J=3-2) Intensity Ratio[C II] 158 µm / CO(J=6-5) Intensity Ratio[C II] 158 µm / 13CO(J=1-0) Intensity Ratio[C II] 158 µm / 13CO(J=6-5) Intensity Ratio
CO(J=2-1) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=4-3) Intensity Ratio
[C I] 609 µm / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=2-1) Intensity Ratio
[C I] 609 µm / 13CO(J=3-2) Intensity RatioCO(J=4-3) / CO(J=2-1) Intensity RatioCO(J=6-5) / CO(J=1-0) Intensity RatioCO(J=7-6) / CO(J=1-0) Intensity Ratio
CO(J=7-6) / CO(J=2-1) Intensity RatioCO(J=7-6) / CO(J=4-3) Intensity RatioCO(J=7-6) / CO(J=5-4) Intensity RatioCO(J=7-6) / CO(J=6-5) Intensity Ratio
CO(J=8-7) / CO(J=5-4) Intensity RatioCO(J=8-7) / CO(J=6-5) Intensity RatioCO(J=9-8) / CO(J=5-4) Intensity RatioCO(J=9-8) / CO(J=6-5) Intensity Ratio
CO(J=10-9) / CO(J=5-4) Intensity RatioCO(J=10-9) / CO(J=6-5) Intensity RatioCO(J=10-9) / CO(J=7-6) Intensity RatioCO(J=11-10) / CO(J=5-4) Intensity Ratio
CO(J=11-10) / CO(J=6-5) Intensity RatioCO(J=11-10) / CO(J=8-7) Intensity RatioCO(J=12-11) / CO(J=5-4) Intensity RatioCO(J=12-11) / CO(J=6-5) Intensity Ratio
CO(J=13-12) / CO(J=5-4) Intensity RatioCO(J=13-12) / CO(J=6-5) Intensity RatioCO(J=14-13) / CO(J=5-4) Intensity RatioCO(J=14-13) / CO(J=6-5) Intensity Ratio
CO(J=15-14) / CO(J=5-4) Intensity RatioCO(J=15-14) / CO(J=6-5) Intensity RatioCO(J=16-15) / CO(J=5-4) Intensity RatioCO(J=16-15) / CO(J=6-5) Intensity Ratio
CO(J=17-16) / CO(J=5-4) Intensity RatioCO(J=17-16) / CO(J=6-5) Intensity RatioCO(J=18-17) / CO(J=5-4) Intensity RatioCO(J=18-17) / CO(J=6-5) Intensity Ratio
13CO(J=1-0) / CO(J=1-0) Intensity Ratio13CO(J=2-1) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / CO(J=2-1) Intensity Ratio13CO(J=4-3) / CO(J=2-1) Intensity Ratio
13CO(J=5-4) / CO(J=2-1) Intensity Ratio13CO(J=6-5) / CO(J=2-1) Intensity Ratio13CO(J=7-6) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio
H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio
H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity RatioH22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio[C I] 370 µm Intensity[C I] 609 µm Intensity
[C II] 158 µm Intensity[O I] 63 µm Intensity[O I] 145 µm IntensityCO(J=1-0) Intensity
CO(J=2-1) IntensityCO(J=3-2) IntensityCO(J=4-3) IntensityCO(J=5-4) Intensity
CO(J=6-5) IntensityCO(J=7-6) IntensityCO(J=8-7) IntensityCO(J=11-10) Intensity
13CO(J=1-0) Intensity13CO(J=2-1) Intensity13CO(J=3-2) IntensityH20-0S(3) 9.7 µm Intensity
H20-0S(2) 12.3 µm IntensityH20-0S(1) 17 µm IntensityH20-0S(0) 28.2 µm IntensityTemperature at AV = 0.01
+

+
+
+ + + + diff --git a/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.fits new file mode 100644 index 00000000..10547b45 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.html b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.html new file mode 100644 index 00000000..859da70d --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) / CO(J=1-0) Intensity Ratio + +
+

+13CO(J=1-0) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.png b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.png new file mode 100644 index 00000000..a875a571 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO10_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO10sm.fits b/models/smc_Z0.2_L75_constant_density/13CO10sm.fits new file mode 100644 index 00000000..b2be5b80 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO10sm.html b/models/smc_Z0.2_L75_constant_density/13CO10sm.html new file mode 100644 index 00000000..3400b1bc --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=1-0) Intensity + +
+

+13CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO10sm.png b/models/smc_Z0.2_L75_constant_density/13CO10sm.png new file mode 100644 index 00000000..aa04b7e6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.fits new file mode 100644 index 00000000..66a2e019 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.html new file mode 100644 index 00000000..7d85e8b9 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=2-1) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.png new file mode 100644 index 00000000..a525e573 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO21_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO21sm.fits new file mode 100644 index 00000000..534b7ada Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO21sm.html new file mode 100644 index 00000000..c6c5bc82 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=2-1) Intensity + +
+

+13CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO21sm.png new file mode 100644 index 00000000..b1464552 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.fits b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.fits new file mode 100644 index 00000000..8b1ea58f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.html b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.html new file mode 100644 index 00000000..b54b69d3 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.png b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.png new file mode 100644 index 00000000..37196256 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32_13CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.fits new file mode 100644 index 00000000..d13c5692 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.html new file mode 100644 index 00000000..68b98486 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.png new file mode 100644 index 00000000..face1b99 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32sm.fits b/models/smc_Z0.2_L75_constant_density/13CO32sm.fits new file mode 100644 index 00000000..4a7f31f3 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO32sm.html b/models/smc_Z0.2_L75_constant_density/13CO32sm.html new file mode 100644 index 00000000..6478f443 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=3-2) Intensity + +
+

+13CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO32sm.png b/models/smc_Z0.2_L75_constant_density/13CO32sm.png new file mode 100644 index 00000000..1a0e6263 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO32sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.fits new file mode 100644 index 00000000..74795ba1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.html new file mode 100644 index 00000000..b9ca5415 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.png new file mode 100644 index 00000000..b0fc96c1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.fits new file mode 100644 index 00000000..26031ac6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.html new file mode 100644 index 00000000..9a83b101 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=5-4) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=5-4) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.png new file mode 100644 index 00000000..7decb021 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO54_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.fits new file mode 100644 index 00000000..71a01220 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.html new file mode 100644 index 00000000..a70c4a2c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=6-5) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=6-5) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.png new file mode 100644 index 00000000..ededd720 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO65_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.fits new file mode 100644 index 00000000..108bb3b2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.html b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.html new file mode 100644 index 00000000..fc3d9449 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + <sup>13</sup>CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+13CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.png b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.png new file mode 100644 index 00000000..17f0ccea Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/13CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.fits b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.fits new file mode 100644 index 00000000..2b3f5239 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.html b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.html new file mode 100644 index 00000000..66cacb34 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm / [C I] 609 µm Intensity Ratio + +
+

+[C I] 370 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.png b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.png new file mode 100644 index 00000000..da335160 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI370_CI609sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI370sm.fits b/models/smc_Z0.2_L75_constant_density/CI370sm.fits new file mode 100644 index 00000000..eb7b5e07 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI370sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI370sm.html b/models/smc_Z0.2_L75_constant_density/CI370sm.html new file mode 100644 index 00000000..df2a2949 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI370sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 370 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 370 µm Intensity + +
+

+[C I] 370 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI370sm.png b/models/smc_Z0.2_L75_constant_density/CI370sm.png new file mode 100644 index 00000000..5617129b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI370sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.fits new file mode 100644 index 00000000..92529345 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.html b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.html new file mode 100644 index 00000000..3f1a6a7d --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.png b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.png new file mode 100644 index 00000000..747ff03a Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.fits new file mode 100644 index 00000000..405d5bb7 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.html b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.html new file mode 100644 index 00000000..090cf887 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.png b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.png new file mode 100644 index 00000000..a69389f2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.fits new file mode 100644 index 00000000..fe05ee8f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.html b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.html new file mode 100644 index 00000000..cd37935d --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / <sup>13</sup>CO(J=3-2) Intensity Ratio + +
+

+[C I] 609 µm / 13CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.png b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.png new file mode 100644 index 00000000..3c333d3f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_13CO32sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.fits new file mode 100644 index 00000000..6b7adfb8 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.html new file mode 100644 index 00000000..3952fec5 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=1-0) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.png new file mode 100644 index 00000000..c434fa33 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.fits new file mode 100644 index 00000000..401885ab Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.html b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.html new file mode 100644 index 00000000..7d59bd5a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=2-1) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.png b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.png new file mode 100644 index 00000000..8ef9ab52 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.fits b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.fits new file mode 100644 index 00000000..8df01bac Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.html b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.html new file mode 100644 index 00000000..7dfa655a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm / CO(J=4-3) Intensity Ratio + +
+

+[C I] 609 µm / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.png b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.png new file mode 100644 index 00000000..5fe28280 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609_CO43sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609sm.fits b/models/smc_Z0.2_L75_constant_density/CI609sm.fits new file mode 100644 index 00000000..230fd41c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CI609sm.html b/models/smc_Z0.2_L75_constant_density/CI609sm.html new file mode 100644 index 00000000..1b77d1e0 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C I] 609 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C I] 609 µm Intensity + +
+

+[C I] 609 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CI609sm.png b/models/smc_Z0.2_L75_constant_density/CI609sm.png new file mode 100644 index 00000000..65c99778 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CI609sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.fits new file mode 100644 index 00000000..8696eec2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.html b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.html new file mode 100644 index 00000000..ec35bb7a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.png b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.png new file mode 100644 index 00000000..89baa0d6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_13CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.fits new file mode 100644 index 00000000..865b1b67 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.html b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.html new file mode 100644 index 00000000..917775ff --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.png b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.png new file mode 100644 index 00000000..7a6b3a3c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_13CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.fits new file mode 100644 index 00000000..45a7ea91 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.html b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.html new file mode 100644 index 00000000..7083bd74 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [C I] 609 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [C I] 609 µm Intensity Ratio + +
+

+[C II] 158 µm / [C I] 609 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.png b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.png new file mode 100644 index 00000000..abcecd9e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CI609sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.fits new file mode 100644 index 00000000..88bc44bf Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.html new file mode 100644 index 00000000..5f42a9d7 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=1-0) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.png new file mode 100644 index 00000000..9a8a007f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.fits new file mode 100644 index 00000000..1f65e1c1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.html b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.html new file mode 100644 index 00000000..c0b810b9 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=2-1) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.png b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.png new file mode 100644 index 00000000..a7b8910f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.fits new file mode 100644 index 00000000..b188b34e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.html b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.html new file mode 100644 index 00000000..88fc9a91 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=3-2) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=3-2) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=3-2) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.png b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.png new file mode 100644 index 00000000..5e0066c2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO32sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.fits new file mode 100644 index 00000000..31ddaad4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.html new file mode 100644 index 00000000..d9ae81a4 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / CO(J=6-5) Intensity Ratio + +
+

+[C II] 158 µm / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.png new file mode 100644 index 00000000..8b958284 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.fits b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.fits new file mode 100644 index 00000000..0a5e80ab Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.html b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.html new file mode 100644 index 00000000..1621eef0 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / I<sub>FIR</sub> Intensity Ratio + +
+

+[C II] 158 µm / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.png b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.png new file mode 100644 index 00000000..11ef0405 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.fits b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.fits new file mode 100644 index 00000000..e38fe42f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.html b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.html new file mode 100644 index 00000000..005056f1 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm / [O I] 145 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm / [O I] 145 µm Intensity Ratio + +
+

+[C II] 158 µm / [O I] 145 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.png b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.png new file mode 100644 index 00000000..da3dc289 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158_OI145sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158sm.fits b/models/smc_Z0.2_L75_constant_density/CII158sm.fits new file mode 100644 index 00000000..bfd30ed9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CII158sm.html b/models/smc_Z0.2_L75_constant_density/CII158sm.html new file mode 100644 index 00000000..11ab8d1e --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[C II] 158 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [C II] 158 µm Intensity + +
+

+[C II] 158 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CII158sm.png b/models/smc_Z0.2_L75_constant_density/CII158sm.png new file mode 100644 index 00000000..8ffa4d8e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CII158sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.fits new file mode 100644 index 00000000..e78cfb12 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.html new file mode 100644 index 00000000..d904b8aa --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.png new file mode 100644 index 00000000..bad7ece4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.fits new file mode 100644 index 00000000..d8ae453b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.html new file mode 100644 index 00000000..98c1eb08 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.png new file mode 100644 index 00000000..717a15b9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.fits b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.fits new file mode 100644 index 00000000..cff0f734 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.html b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.html new file mode 100644 index 00000000..6a044d91 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=10-9) / CO(J=7-6) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=10-9) / CO(J=7-6) Intensity Ratio + +
+

+CO(J=10-9) / CO(J=7-6) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.png b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.png new file mode 100644 index 00000000..1823c5ad Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO109_CO76sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CO10sm.fits new file mode 100644 index 00000000..8a3bcecb Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO10sm.html b/models/smc_Z0.2_L75_constant_density/CO10sm.html new file mode 100644 index 00000000..f35155e5 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=1-0) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=1-0) Intensity + +
+

+CO(J=1-0) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO10sm.png b/models/smc_Z0.2_L75_constant_density/CO10sm.png new file mode 100644 index 00000000..590a9af3 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.fits new file mode 100644 index 00000000..ebce4903 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.html new file mode 100644 index 00000000..8fad7bef --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.png new file mode 100644 index 00000000..bc4fbdd1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.fits new file mode 100644 index 00000000..dc81a651 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.html new file mode 100644 index 00000000..7cd06ea6 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.png new file mode 100644 index 00000000..1a1ee9e9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.fits b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.fits new file mode 100644 index 00000000..d71cd9bb Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.html b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.html new file mode 100644 index 00000000..d2b9616f --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) / CO(J=8-7) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) / CO(J=8-7) Intensity Ratio + +
+

+CO(J=11-10) / CO(J=8-7) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.png b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.png new file mode 100644 index 00000000..eaefd656 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110_CO87sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110sm.fits b/models/smc_Z0.2_L75_constant_density/CO1110sm.fits new file mode 100644 index 00000000..ba7c4498 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1110sm.html b/models/smc_Z0.2_L75_constant_density/CO1110sm.html new file mode 100644 index 00000000..5f5613ae --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1110sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=11-10) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=11-10) Intensity + +
+

+CO(J=11-10) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1110sm.png b/models/smc_Z0.2_L75_constant_density/CO1110sm.png new file mode 100644 index 00000000..bc7991ea Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1110sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.fits new file mode 100644 index 00000000..36c5788f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.html new file mode 100644 index 00000000..d9383d07 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.png new file mode 100644 index 00000000..79fa6ed3 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1211_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.fits new file mode 100644 index 00000000..5a9698e1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.html new file mode 100644 index 00000000..2b2d05ed --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=12-11) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=12-11) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=12-11) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.png new file mode 100644 index 00000000..e49a48fe Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1211_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.fits new file mode 100644 index 00000000..6fc4e4f7 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.html new file mode 100644 index 00000000..408d97b0 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.png new file mode 100644 index 00000000..a9e5677b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1312_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.fits new file mode 100644 index 00000000..e87ad79b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.html new file mode 100644 index 00000000..fb36eff6 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=13-12) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=13-12) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=13-12) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.png new file mode 100644 index 00000000..25df148b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1312_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.fits new file mode 100644 index 00000000..61cd394e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.html new file mode 100644 index 00000000..ddef3ea0 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.png new file mode 100644 index 00000000..5207b892 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1413_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.fits new file mode 100644 index 00000000..29c5c48f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.html new file mode 100644 index 00000000..7267ffd4 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=14-13) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=14-13) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=14-13) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.png new file mode 100644 index 00000000..9db90e0a Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1413_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.fits new file mode 100644 index 00000000..3ded5ff0 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.html new file mode 100644 index 00000000..4dcb37b6 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.png new file mode 100644 index 00000000..9d5a01c9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1514_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.fits new file mode 100644 index 00000000..6a8a96a4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.html new file mode 100644 index 00000000..bfc34f72 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=15-14) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=15-14) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=15-14) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.png new file mode 100644 index 00000000..a6df4090 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1514_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.fits new file mode 100644 index 00000000..bdf87bb2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.html new file mode 100644 index 00000000..d54f3d6a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.png new file mode 100644 index 00000000..63d08778 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1615_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.fits new file mode 100644 index 00000000..585e7deb Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.html new file mode 100644 index 00000000..4198f999 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=16-15) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=16-15) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=16-15) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.png new file mode 100644 index 00000000..44fd78e2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1615_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.fits new file mode 100644 index 00000000..6dc3628a Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.html new file mode 100644 index 00000000..d85d5e71 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.png new file mode 100644 index 00000000..099bbc43 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1716_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.fits new file mode 100644 index 00000000..e43b9d3b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.html new file mode 100644 index 00000000..cf802e3f --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=17-16) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=17-16) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=17-16) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.png new file mode 100644 index 00000000..e7f21808 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1716_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.fits new file mode 100644 index 00000000..2ced1608 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.html new file mode 100644 index 00000000..37cd7ca9 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.png new file mode 100644 index 00000000..f8aab891 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1817_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.fits new file mode 100644 index 00000000..3a955b10 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.html new file mode 100644 index 00000000..2e2f809a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=18-17) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=18-17) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=18-17) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.png new file mode 100644 index 00000000..d522a064 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO1817_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.fits new file mode 100644 index 00000000..3d32e49e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.html new file mode 100644 index 00000000..79e8df58 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=2-1) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.png new file mode 100644 index 00000000..16f06aec Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO21_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CO21sm.fits new file mode 100644 index 00000000..9aecd788 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO21sm.html b/models/smc_Z0.2_L75_constant_density/CO21sm.html new file mode 100644 index 00000000..4646d5e4 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=2-1) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=2-1) Intensity + +
+

+CO(J=2-1) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO21sm.png b/models/smc_Z0.2_L75_constant_density/CO21sm.png new file mode 100644 index 00000000..42d1ddc5 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.fits new file mode 100644 index 00000000..b77231e4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.html new file mode 100644 index 00000000..bb32b7cc --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.png new file mode 100644 index 00000000..e5185d3f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.fits new file mode 100644 index 00000000..05e9ccf0 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.html b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.html new file mode 100644 index 00000000..09a6e003 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=3-2) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.png b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.png new file mode 100644 index 00000000..eafa0d86 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32sm.fits b/models/smc_Z0.2_L75_constant_density/CO32sm.fits new file mode 100644 index 00000000..f4f33a9c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO32sm.html b/models/smc_Z0.2_L75_constant_density/CO32sm.html new file mode 100644 index 00000000..1e234e2c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO32sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=3-2) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=3-2) Intensity + +
+

+CO(J=3-2) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO32sm.png b/models/smc_Z0.2_L75_constant_density/CO32sm.png new file mode 100644 index 00000000..d24eae18 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO32sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.fits new file mode 100644 index 00000000..acd64ae6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.html b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.html new file mode 100644 index 00000000..221b58d6 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=4-3) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.png b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.png new file mode 100644 index 00000000..78630945 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO43_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO43sm.fits b/models/smc_Z0.2_L75_constant_density/CO43sm.fits new file mode 100644 index 00000000..74666680 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO43sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO43sm.html b/models/smc_Z0.2_L75_constant_density/CO43sm.html new file mode 100644 index 00000000..0403d8bd --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=4-3) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=4-3) Intensity + +
+

+CO(J=4-3) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO43sm.png b/models/smc_Z0.2_L75_constant_density/CO43sm.png new file mode 100644 index 00000000..0b56f34a Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO43sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO54sm.fits new file mode 100644 index 00000000..d6f73658 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO54sm.html new file mode 100644 index 00000000..ac297f01 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=5-4) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=5-4) Intensity + +
+

+CO(J=5-4) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO54sm.png new file mode 100644 index 00000000..ada3edf9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.fits new file mode 100644 index 00000000..256f475d Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.html new file mode 100644 index 00000000..84d743b7 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=6-5) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.png new file mode 100644 index 00000000..fc4b7817 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO65_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO65sm.fits new file mode 100644 index 00000000..b650815f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO65sm.html new file mode 100644 index 00000000..842ee2bf --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=6-5) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=6-5) Intensity + +
+

+CO(J=6-5) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO65sm.png new file mode 100644 index 00000000..e7f849f9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.fits b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.fits new file mode 100644 index 00000000..597db5b9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.html b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.html new file mode 100644 index 00000000..9325735c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=1-0) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=1-0) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=1-0) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.png b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.png new file mode 100644 index 00000000..578533ec Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO10sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.fits b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.fits new file mode 100644 index 00000000..0ad133fe Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.html b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.html new file mode 100644 index 00000000..70d1ef4f --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=2-1) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=2-1) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=2-1) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.png b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.png new file mode 100644 index 00000000..71547470 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO21sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.fits b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.fits new file mode 100644 index 00000000..90844174 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.html b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.html new file mode 100644 index 00000000..627f4b81 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=4-3) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=4-3) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=4-3) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.png b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.png new file mode 100644 index 00000000..cc53b98f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO43sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.fits new file mode 100644 index 00000000..1645047c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.html new file mode 100644 index 00000000..b627d316 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.png new file mode 100644 index 00000000..9277b4ad Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.fits new file mode 100644 index 00000000..c0da6dc2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.html new file mode 100644 index 00000000..9d12f29c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=7-6) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.png new file mode 100644 index 00000000..307af32f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76sm.fits b/models/smc_Z0.2_L75_constant_density/CO76sm.fits new file mode 100644 index 00000000..5cd98512 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO76sm.html b/models/smc_Z0.2_L75_constant_density/CO76sm.html new file mode 100644 index 00000000..829bf16a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO76sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=7-6) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=7-6) Intensity + +
+

+CO(J=7-6) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO76sm.png b/models/smc_Z0.2_L75_constant_density/CO76sm.png new file mode 100644 index 00000000..a0540425 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO76sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.fits new file mode 100644 index 00000000..764b9feb Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.html new file mode 100644 index 00000000..bd7d5da5 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.png new file mode 100644 index 00000000..6ce5ebb3 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.fits new file mode 100644 index 00000000..55630c44 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.html new file mode 100644 index 00000000..94c4025c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=8-7) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.png new file mode 100644 index 00000000..b7beb860 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87sm.fits b/models/smc_Z0.2_L75_constant_density/CO87sm.fits new file mode 100644 index 00000000..5fa841c9 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO87sm.html b/models/smc_Z0.2_L75_constant_density/CO87sm.html new file mode 100644 index 00000000..2bb81242 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO87sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=8-7) Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=8-7) Intensity + +
+

+CO(J=8-7) Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO87sm.png b/models/smc_Z0.2_L75_constant_density/CO87sm.png new file mode 100644 index 00000000..a4b982f5 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO87sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.fits b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.fits new file mode 100644 index 00000000..5d63b642 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.html b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.html new file mode 100644 index 00000000..c5b4bcc3 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=5-4) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=5-4) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=5-4) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.png b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.png new file mode 100644 index 00000000..7aa954f0 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO98_CO54sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.fits b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.fits new file mode 100644 index 00000000..e9ce72a4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.html b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.html new file mode 100644 index 00000000..be96c72e --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+CO(J=9-8) / CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + CO(J=9-8) / CO(J=6-5) Intensity Ratio + +
+

+CO(J=9-8) / CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.png b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.png new file mode 100644 index 00000000..aec02126 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/CO98_CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S0sm.fits b/models/smc_Z0.2_L75_constant_density/H200S0sm.fits new file mode 100644 index 00000000..902e517e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S0sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S0sm.html b/models/smc_Z0.2_L75_constant_density/H200S0sm.html new file mode 100644 index 00000000..de65f731 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(0) 28.2 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(0) 28.2 µm Intensity + +
+

+H20-0S(0) 28.2 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S0sm.png b/models/smc_Z0.2_L75_constant_density/H200S0sm.png new file mode 100644 index 00000000..c7f2c951 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S0sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S1sm.fits b/models/smc_Z0.2_L75_constant_density/H200S1sm.fits new file mode 100644 index 00000000..6a1fc51e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S1sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S1sm.html b/models/smc_Z0.2_L75_constant_density/H200S1sm.html new file mode 100644 index 00000000..759f6914 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(1) 17 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(1) 17 µm Intensity + +
+

+H20-0S(1) 17 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S1sm.png b/models/smc_Z0.2_L75_constant_density/H200S1sm.png new file mode 100644 index 00000000..7c1a7b63 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S1sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.fits b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.fits new file mode 100644 index 00000000..f3b63bf0 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.html b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.html new file mode 100644 index 00000000..0522f49c --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.png b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.png new file mode 100644 index 00000000..7ea26a31 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2_H200S0sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.fits b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.fits new file mode 100644 index 00000000..19abf0d2 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.html b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.html new file mode 100644 index 00000000..e4925e5b --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.png b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.png new file mode 100644 index 00000000..131ad5fe Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2_H200S1sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2sm.fits b/models/smc_Z0.2_L75_constant_density/H200S2sm.fits new file mode 100644 index 00000000..761c4ed1 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S2sm.html b/models/smc_Z0.2_L75_constant_density/H200S2sm.html new file mode 100644 index 00000000..b6314b5e --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(2) 12.3 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(2) 12.3 µm Intensity + +
+

+H20-0S(2) 12.3 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S2sm.png b/models/smc_Z0.2_L75_constant_density/H200S2sm.png new file mode 100644 index 00000000..9a563f1f Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S2sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.fits b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.fits new file mode 100644 index 00000000..8cff0416 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.html b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.html new file mode 100644 index 00000000..d3e5e689 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(0) 28.2 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.png b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.png new file mode 100644 index 00000000..99536ab6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S0sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.fits b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.fits new file mode 100644 index 00000000..8b2a94a6 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.html b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.html new file mode 100644 index 00000000..0789f18d --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(1) 17 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.png b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.png new file mode 100644 index 00000000..f94c3526 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S1sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.fits b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.fits new file mode 100644 index 00000000..fa47cd17 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.html b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.html new file mode 100644 index 00000000..cba91682 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm / H<sub>2</sub>0-0S(2) 12.3 µm Intensity Ratio + +
+

+H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.png b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.png new file mode 100644 index 00000000..98c72c7c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3_H200S2sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3sm.fits b/models/smc_Z0.2_L75_constant_density/H200S3sm.fits new file mode 100644 index 00000000..7829c71c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H200S3sm.html b/models/smc_Z0.2_L75_constant_density/H200S3sm.html new file mode 100644 index 00000000..93099b66 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H200S3sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H20-0S(3) 9.7 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>0-0S(3) 9.7 µm Intensity + +
+

+H20-0S(3) 9.7 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H200S3sm.png b/models/smc_Z0.2_L75_constant_density/H200S3sm.png new file mode 100644 index 00000000..306dd821 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H200S3sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.fits b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.fits new file mode 100644 index 00000000..ed8b9f4d Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.html b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.html new file mode 100644 index 00000000..1ee32aa1 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + H<sub>2</sub>2-1S(1) 2.24 µm / H<sub>2</sub>1-0S(1) 2.12 µm Intensity Ratio + +
+

+H22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.png b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.png new file mode 100644 index 00000000..33dcbc25 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/H221S1_H210S1sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.fits b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.fits new file mode 100644 index 00000000..b00f7ea0 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.html b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.html new file mode 100644 index 00000000..87e3fb1f --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 145 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.png b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.png new file mode 100644 index 00000000..8b28ec7e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.fits b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.fits new file mode 100644 index 00000000..726c0de4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.html b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.html new file mode 100644 index 00000000..04b9f39e --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 145 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.png b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.png new file mode 100644 index 00000000..c24a981c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145_13CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.fits b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.fits new file mode 100644 index 00000000..2c1cabd5 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.html b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.html new file mode 100644 index 00000000..d7f8300e --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm / [O I] 63 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm / [O I] 63 µm Intensity Ratio + +
+

+[O I] 145 µm / [O I] 63 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.png b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.png new file mode 100644 index 00000000..0c4c876d Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145_OI63sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145sm.fits b/models/smc_Z0.2_L75_constant_density/OI145sm.fits new file mode 100644 index 00000000..5ac350e8 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI145sm.html b/models/smc_Z0.2_L75_constant_density/OI145sm.html new file mode 100644 index 00000000..1875fedc --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI145sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 145 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 145 µm Intensity + +
+

+[O I] 145 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI145sm.png b/models/smc_Z0.2_L75_constant_density/OI145sm.png new file mode 100644 index 00000000..f02f8d4b Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI145sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.fits b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.fits new file mode 100644 index 00000000..f4269e7d Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.html b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.html new file mode 100644 index 00000000..eb63fb07 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + ([O I] 63 µm + [C II] 158 µm) / I<sub>FIR</sub> Intensity Ratio + +
+

+([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.png b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.png new file mode 100644 index 00000000..19c9a70c Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63+CII158_FIRsm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.fits b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.fits new file mode 100644 index 00000000..b1dec79e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.html b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.html new file mode 100644 index 00000000..dd9f1ef8 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / <sup>13</sup>CO(J=6-5) Intensity Ratio + +
+

+[O I] 63 µm / 13CO(J=6-5) Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.png b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.png new file mode 100644 index 00000000..bb741b87 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63_13CO65sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.fits b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.fits new file mode 100644 index 00000000..82c06bc5 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.html b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.html new file mode 100644 index 00000000..b9ea97e1 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm / [C II] 158 µm Intensity Ratio +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm / [C II] 158 µm Intensity Ratio + +
+

+[O I] 63 µm / [C II] 158 µm Intensity Ratio emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.png b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.png new file mode 100644 index 00000000..09909c2e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63_CII158sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63sm.fits b/models/smc_Z0.2_L75_constant_density/OI63sm.fits new file mode 100644 index 00000000..d940fc3e Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/OI63sm.html b/models/smc_Z0.2_L75_constant_density/OI63sm.html new file mode 100644 index 00000000..5ec2f710 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/OI63sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+[O I] 63 µm Intensity +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + [O I] 63 µm Intensity + +
+

+[O I] 63 µm Intensity emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/OI63sm.png b/models/smc_Z0.2_L75_constant_density/OI63sm.png new file mode 100644 index 00000000..a5202c8d Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/OI63sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.fits b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.fits new file mode 100644 index 00000000..e8e9e3c4 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.fits differ diff --git a/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.html b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.html new file mode 100644 index 00000000..7a03763a --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.html @@ -0,0 +1,66 @@ + + + + + + +
+
+ +

+Temperature at AV = 0.01 +

+

pdrtpy ModelSet: smc

+
+
+
+
+
+
+
+ + Temperature at A<sub>V</sub> = 0.01 + +
+

+Temperature at AV = 0.01 emitted from the surface of a PDR +as a function of the cloud density n and the FUV flux incident on the cloud G0. +The above model is at a viewing angle of i=75 degrees, where i=0 is face-on. +The models in the smc ModelSet are based on Kaufman et al. 2006 , Wolfire et al. 2010, and Neufeld & Wolfire 2016. They use z=0.2 and these parameters. More details are in the FITS headers. +

+The FITS file is available for download. +

+
+
+
+
+
+ + + + + + + \ No newline at end of file diff --git a/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.png b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.png new file mode 100644 index 00000000..a44a6722 Binary files /dev/null and b/models/smc_Z0.2_L75_constant_density/TSAV0p01sm.png differ diff --git a/models/smc_Z0.2_L75_constant_density/index.html b/models/smc_Z0.2_L75_constant_density/index.html new file mode 100644 index 00000000..31dd2999 --- /dev/null +++ b/models/smc_Z0.2_L75_constant_density/index.html @@ -0,0 +1,73 @@ + + + + + + + + + +
+
+ +

+Wolfire/Kaufman 2020 Small Magellanic Cloud, AV=7, Dust abundance=0.1, no freeze-out, Z=0.2, losangle=75

+

+Below are links to the individual FITS files +and plots in the smc z=0.2 losangle=75 ModelSet. We also provide a gzipped tarball of all the smc FITS and PNG files. + + + + + + + + + + + + + + + + + + + + + + + + + +
[O I] 63 µm / [C II] 158 µm Intensity Ratio[O I] 63 µm / 13CO(J=6-5) Intensity Ratio([O I] 63 µm + [C II] 158 µm) / IFIR Intensity Ratio([O I] 145 µm + [C II] 158 µm) / IFIR Intensity Ratio
[O I] 145 µm / [O I] 63 µm Intensity Ratio[O I] 145 µm / 13CO(J=6-5) Intensity Ratio[C I] 370 µm / [C I] 609 µm Intensity Ratio[C II] 158 µm / [C I] 609 µm Intensity Ratio
[C II] 158 µm / [O I] 145 µm Intensity Ratio[C II] 158 µm / IFIR Intensity Ratio[C II] 158 µm / CO(J=1-0) Intensity Ratio[C II] 158 µm / CO(J=2-1) Intensity Ratio
[C II] 158 µm / CO(J=3-2) Intensity Ratio[C II] 158 µm / CO(J=6-5) Intensity Ratio[C II] 158 µm / 13CO(J=1-0) Intensity Ratio[C II] 158 µm / 13CO(J=6-5) Intensity Ratio
CO(J=2-1) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=1-0) Intensity RatioCO(J=3-2) / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=4-3) Intensity Ratio
[C I] 609 µm / CO(J=2-1) Intensity Ratio[C I] 609 µm / CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=1-0) Intensity Ratio[C I] 609 µm / 13CO(J=2-1) Intensity Ratio
[C I] 609 µm / 13CO(J=3-2) Intensity RatioCO(J=4-3) / CO(J=2-1) Intensity RatioCO(J=6-5) / CO(J=1-0) Intensity RatioCO(J=7-6) / CO(J=1-0) Intensity Ratio
CO(J=7-6) / CO(J=2-1) Intensity RatioCO(J=7-6) / CO(J=4-3) Intensity RatioCO(J=7-6) / CO(J=5-4) Intensity RatioCO(J=7-6) / CO(J=6-5) Intensity Ratio
CO(J=8-7) / CO(J=5-4) Intensity RatioCO(J=8-7) / CO(J=6-5) Intensity RatioCO(J=9-8) / CO(J=5-4) Intensity RatioCO(J=9-8) / CO(J=6-5) Intensity Ratio
CO(J=10-9) / CO(J=5-4) Intensity RatioCO(J=10-9) / CO(J=6-5) Intensity RatioCO(J=10-9) / CO(J=7-6) Intensity RatioCO(J=11-10) / CO(J=5-4) Intensity Ratio
CO(J=11-10) / CO(J=6-5) Intensity RatioCO(J=11-10) / CO(J=8-7) Intensity RatioCO(J=12-11) / CO(J=5-4) Intensity RatioCO(J=12-11) / CO(J=6-5) Intensity Ratio
CO(J=13-12) / CO(J=5-4) Intensity RatioCO(J=13-12) / CO(J=6-5) Intensity RatioCO(J=14-13) / CO(J=5-4) Intensity RatioCO(J=14-13) / CO(J=6-5) Intensity Ratio
CO(J=15-14) / CO(J=5-4) Intensity RatioCO(J=15-14) / CO(J=6-5) Intensity RatioCO(J=16-15) / CO(J=5-4) Intensity RatioCO(J=16-15) / CO(J=6-5) Intensity Ratio
CO(J=17-16) / CO(J=5-4) Intensity RatioCO(J=17-16) / CO(J=6-5) Intensity RatioCO(J=18-17) / CO(J=5-4) Intensity RatioCO(J=18-17) / CO(J=6-5) Intensity Ratio
13CO(J=1-0) / CO(J=1-0) Intensity Ratio13CO(J=2-1) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / CO(J=2-1) Intensity Ratio13CO(J=4-3) / CO(J=2-1) Intensity Ratio
13CO(J=5-4) / CO(J=2-1) Intensity Ratio13CO(J=6-5) / CO(J=2-1) Intensity Ratio13CO(J=7-6) / CO(J=2-1) Intensity Ratio13CO(J=3-2) / 13CO(J=1-0) Intensity Ratio
H20-0S(2) 12.3 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(2) 12.3 µm / H20-0S(1) 17 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(0) 28.2 µm Intensity RatioH20-0S(3) 9.7 µm / H20-0S(1) 17 µm Intensity Ratio
H20-0S(3) 9.7 µm / H20-0S(2) 12.3 µm Intensity RatioH22-1S(1) 2.24 µm / H21-0S(1) 2.12 µm Intensity Ratio[C I] 370 µm Intensity[C I] 609 µm Intensity
[C II] 158 µm Intensity[O I] 63 µm Intensity[O I] 145 µm IntensityCO(J=1-0) Intensity
CO(J=2-1) IntensityCO(J=3-2) IntensityCO(J=4-3) IntensityCO(J=5-4) Intensity
CO(J=6-5) IntensityCO(J=7-6) IntensityCO(J=8-7) IntensityCO(J=11-10) Intensity
13CO(J=1-0) Intensity13CO(J=2-1) Intensity13CO(J=3-2) IntensityH20-0S(3) 9.7 µm Intensity
H20-0S(2) 12.3 µm IntensityH20-0S(1) 17 µm IntensityH20-0S(0) 28.2 µm IntensityTemperature at AV = 0.01
+

+
+
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+++ b/models/wk2020_Z1.0_L0_constant_density/index.html @@ -33,10 +33,10 @@

-Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=0

+Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=0, avlos=7.00

Below are links to the individual FITS files -and plots in the wk2020 wk2020 z=1.0 losangle=0 ModelSet. We also provide a gzipped tarball of all the wk2020 FITS and PNG files. diff --git a/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.fits b/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.fits index 8aafbeb4..20d4c628 100644 Binary files a/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.fits and b/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.fits differ diff --git a/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.png b/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.png index 880834db..fb5fd3f0 100644 Binary files a/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.png and b/models/wk2020_Z1.0_L30_constant_density/13CO10_CO10sm.png differ diff --git a/models/wk2020_Z1.0_L30_constant_density/13CO10sm.fits b/models/wk2020_Z1.0_L30_constant_density/13CO10sm.fits index e46761cf..86d25473 100644 Binary files a/models/wk2020_Z1.0_L30_constant_density/13CO10sm.fits and b/models/wk2020_Z1.0_L30_constant_density/13CO10sm.fits differ diff --git 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b/models/wk2020_Z1.0_L30_constant_density/TSAV0p01sm.png index 3705bc65..ff6fbc53 100644 Binary files a/models/wk2020_Z1.0_L30_constant_density/TSAV0p01sm.png and b/models/wk2020_Z1.0_L30_constant_density/TSAV0p01sm.png differ diff --git a/models/wk2020_Z1.0_L30_constant_density/index.html b/models/wk2020_Z1.0_L30_constant_density/index.html index aeeded7c..5bd8511e 100644 --- a/models/wk2020_Z1.0_L30_constant_density/index.html +++ b/models/wk2020_Z1.0_L30_constant_density/index.html @@ -33,10 +33,10 @@

-Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=30

+Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=30, avlos=8.08, avperp=4.04

Below are links to the individual FITS files -and plots in the wk2020 wk2020 z=1.0 losangle=30 ModelSet. We also provide a gzipped tarball of all the wk2020 FITS and PNG files.

diff --git a/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.fits b/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.fits index 1468f746..d24dc788 100644 Binary files a/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.fits and b/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.fits differ diff --git a/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.png b/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.png index a36ba3ec..0e332fad 100644 Binary files a/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.png and b/models/wk2020_Z1.0_L45_constant_density/13CO10_CO10sm.png differ diff --git a/models/wk2020_Z1.0_L45_constant_density/13CO10sm.fits b/models/wk2020_Z1.0_L45_constant_density/13CO10sm.fits index b888e6e0..9f549252 100644 Binary files a/models/wk2020_Z1.0_L45_constant_density/13CO10sm.fits and b/models/wk2020_Z1.0_L45_constant_density/13CO10sm.fits differ diff --git a/models/wk2020_Z1.0_L45_constant_density/13CO10sm.png 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b/models/wk2020_Z1.0_L45_constant_density/TSAV0p01sm.png index 3705bc65..ff6fbc53 100644 Binary files a/models/wk2020_Z1.0_L45_constant_density/TSAV0p01sm.png and b/models/wk2020_Z1.0_L45_constant_density/TSAV0p01sm.png differ diff --git a/models/wk2020_Z1.0_L45_constant_density/index.html b/models/wk2020_Z1.0_L45_constant_density/index.html index c10c83c9..b5e2a6a4 100644 --- a/models/wk2020_Z1.0_L45_constant_density/index.html +++ b/models/wk2020_Z1.0_L45_constant_density/index.html @@ -33,10 +33,10 @@

-Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=45

+Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=45, avlos=9.90, avperp=7.00

Below are links to the individual FITS files -and plots in the wk2020 wk2020 z=1.0 losangle=45 ModelSet. We also provide a gzipped tarball of all the wk2020 FITS and PNG files.

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b/models/wk2020_Z1.0_L60_constant_density/TSAV0p01sm.png index 3705bc65..ff6fbc53 100644 Binary files a/models/wk2020_Z1.0_L60_constant_density/TSAV0p01sm.png and b/models/wk2020_Z1.0_L60_constant_density/TSAV0p01sm.png differ diff --git a/models/wk2020_Z1.0_L60_constant_density/index.html b/models/wk2020_Z1.0_L60_constant_density/index.html index 50f66132..95cdde2a 100644 --- a/models/wk2020_Z1.0_L60_constant_density/index.html +++ b/models/wk2020_Z1.0_L60_constant_density/index.html @@ -33,10 +33,10 @@

-Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=60

+Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=60, avlos=14.00, avperp=12.12

Below are links to the individual FITS files -and plots in the wk2020 wk2020 z=1.0 losangle=60 ModelSet. We also provide a gzipped tarball of all the wk2020 FITS and PNG files.

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-Wolfire/Kaufman 2020 constant density models, AV=7, no freeze-out, Z=1.0, losangle=75

+Wolfire/Kaufman 2020 constant density models, AV=7, Dust abundance=0.1, no freeze-out, Z=1.0, losangle=75, avlos=27.05, avperp=26.12

Below are links to the individual FITS files -and plots in the wk2020 wk2020 z=1.0 losangle=75 ModelSet. We also provide a gzipped tarball of all the wk2020 FITS and PNG files.