Add slitless spectroscopic features#34
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Attempt 1. Likely buggy. This duplicates the class in https://github.com/Roman-Supernova-PIT/galsim-slitless-spec/blob/main/slitlessspec.py.
arunkannawadi
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May 20, 2025
| if ob['filter'] == "H158": | ||
| self.ob['filter'] = "SNPrism" | ||
| else: | ||
| self.ob['filter'] = ob['filter'] |
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If I recall correctly, there is no observing sequence information on the non-imaging bands. If we need to pretend some other band/flux from that band to be the one for prism bands, we need a better solution.
| return SlitlessSpec(**kwargs) | ||
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| RegisterPhotonOpType('SlitlessSpec', SlitlessSpecBuilder()) | ||
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We should merge this with https://github.com/Roman-Supernova-PIT/galsim-slitless-spec/blob/main/slitlessspec.py instead of duplicating it.
He did three things: 1. got the code to work equally well for prism or grism 2. included a new method to compute the dispersion (ie. dlam/dr, where dr is the path along the trace)cleaned up a few things regarding how they do intermediate trsnforms for the wavelength. Long story, but tl;dr is they use dy = polynomial(log10(lambda)) 3. generalized a bit the function log10() so that we can use different transformations.
Implement Grism PhotonOps
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superceded by #73 . Closing this, but keeping the branch alive for now. |
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This needs some removal of hacks and versioning of skyCatalogs before it's deemed fully supported.