deletions | additions       diff --git a/Comparison.tex b/Comparison.tex  index 7a9dd01..e3325d8 100644  --- a/Comparison.tex  +++ b/Comparison.tex 
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\subsection{Kinematic Comparisons}  \begin{table*} \begin{table}  \centering  \begin{tabular}{lllllllll}  \hline \hline 
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\label{tab:chis}  \end{tabular}  \caption{$\chi ^2$ and reduced $\chi ^2$ for various statistical samples of models described in text. Disk models (i.e. M31-like models, including the model based on M31 iteself) are disfavored relative to our COP model or the simple isotropic case.}  \end{table*} \end{table}  In Table \ref{tab:chis} we present our analysis of the $\chi ^2$ values describing the goodness of fit for several statistical samples of modelled systems. We first quote the statistics considering only $\alpha \lt 45^{\circ}$, corresponding to systems with satellites in close to oppositely aligned configurations. We then give the $\chi ^2$ for the full domain, $0^{\circ} \lt \alpha \lt 180^{\circ}$. The $\chi ^2$ are displayed this way in order to illustrate how the picture changes when full domain of $\alpha$ is considered, as in Figures \ref{fig:full} and Figure \ref{fig:zoom}.