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%While the relation between $\mstar$ and subhalo $\mpeak$ for dwarf galaxies remains highly uncertain, likely with significant scatter, in this work the relation is important \emph{only} in assigning infall time distributions to satellites in a 1-dex bin of $\mstar$.  %As \citet{Wetzel2015} showed, satellite infall times generally change by $<10-20\%$ over $\sim 1$ dex in $\mstar$.  See \citet{GarrisonKimmel2014} for more details on ELVIS, and \citet{Wetzel2015} for For  more details on ELVIS and/or  satellite infall times. times, see \citet{GarrisonKimmel2014} and/or \citet{Wetzel2015}.