deletions | additions       diff --git a/quenching_time.tex b/quenching_time.tex  index 3629611..12155da 100644  --- a/quenching_time.tex  +++ b/quenching_time.tex 
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\subsection{Inferred Environmental Quenching Timescales}  We only examine satellites in the simulation out to the maximum distance that they are observed from the MW or M31 in \emph{each} $\mstar$ bin.  (We do take into account the maximum observed distance of dwarfs at each $\mstar$ bin when  The timescale from \citet{Wheeler2014} is based on combining the the galaxy catalog from \citet{Geha2012} with satellite virial-infall times in the Millennium II simulation.  In particular, \citet{Wheeler2014} used a subset of satellites from \citet{Geha2012} at $8.25 < log(\mstar/\msun) < 8.75$ and $9.25 < log(\mstar/\msun) < 9.65$.