deletions | additions       diff --git a/figures/qu.frac_v_m.star_lg_mw_m31_gas.ratio.0.1/caption.tex b/figures/qu.frac_v_m.star_lg_mw_m31_gas.ratio.0.1/caption.tex  index 3beaa94..658785e 100644  --- a/figures/qu.frac_v_m.star_lg_mw_m31_gas.ratio.0.1/caption.tex  +++ b/figures/qu.frac_v_m.star_lg_mw_m31_gas.ratio.0.1/caption.tex 
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For all observed satellites dwarf galaxies within $300\kpc$ of the Milky Way (MW) or Andromeda (M31), the fraction that are quiescent ($\mgas/\mstar<0.1$) versus stellar mass, $\mstar$.  Blue circles show all satellites, violet squares (green triangles) show those of just the MW (M31).  Of these 56 satellites, only 4 are star-forming/gas-rich: LMC ($\mstar=1.5\times10^9\msun$) and SMC ($\mstar=4.6\times10^8\msun$) around the MW, LGS 3 ($\mstar=9.6\times10^5\msun$) and IC 10 ($\mstar=9\times10^7$) ($\mstar=9\times10^7\msun$)  around M31. At $\mstar<8\times10^7\msun$, 50 of 51 satellites are quiescent, and at $\mstar<9\times10^5\msun$ \emph{all} are quiescent.  Error bars show 68\% uncertainty based on the observed counts.