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@@ -7,31 +7,4 @@ Project Lead: Alex Ji (alexji@mit.edu)
Here is the poster presented at University of Michigan Local Group Astrostatistics Conference: PDF
-A paper is in preparation, expected submission in late June. In the meantime, here are some additional plots that were of interest to people at the conference.
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-## Radial Profiles
-Satellite position radial profiles compared to the 11 classical Milky Way satellites.
-The colored lines correspond to different choices of satellites. Blue lines are the first 11 satellites by Vpeak, Green lines are satellites with stellar mass > 10^5.5 Msun, Red lines are satellites with stellar mass > 10^5 Msun. Stellar masses found by Moster et al. 2013 abundance matching.
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-## Orbital alignment with plane
-Here we plot the cumulative number of satellites whose angular momentum is within a certain angle of the plane's minor axis. Solid lines indicate total number pointing in either direction (i.e. co-rotating and anti-co-rotating). Dashed lines indicate total number pointing in single direction.
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-## Edge-On and Face-On Satellite Distributions
-Here are the spatial positions of the satellites relative to the best-fit plane. The colored dots are satellites with stellar mass > 10^5 Msun (the red lines in previous plots). Arrows indicate where the satellite will travel in 1Myr given its current velocity.
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+A paper is in preparation, expected submission in late June.