deletions | additions       diff --git a/section_Previous_measurements_citet_JIMMY13__.tex b/section_Previous_measurements_citet_JIMMY13__.tex  index 4864ade..dd6708f 100644  --- a/section_Previous_measurements_citet_JIMMY13__.tex  +++ b/section_Previous_measurements_citet_JIMMY13__.tex 
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\end{equation}  Where M$_{\rm 20}$ is the 2nd order moment of the brightest 20~per~cent of pixels, and G is the Gini coefficient. In the case of gas-poor galaxies like our sample, a galaxy will be above the threshold if it is currently merging or has merged in the last 0.2~Gyr \citep{LOTZ11}. 4 of the BCGs in the sample are merging. The relevant kinematic and photometric results of \citet{JIMMY13} are presented in Table \ref{tab:kin}.  \begin{table}  \begin{minipage}{0.85\linewidth}\label{sec:phot}  \caption{Kinematic properties of BCGs and their companions from \citet{JIMMY13}. Seven of the BCGs are slow rotating (SR) and two are fast rotating (FR). Four of the BCGs show photometric signs of merging.}  \begin{tabular}{lccccc}  \label{tab:kin} 
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1048C& 0.074 &10.54&1.24&y&FR\\  \hline  \medskip  \caption{Kinematic properties of BCGs and their companions from \citet{JIMMY13}. Seven of the BCGs are slow rotating (SR) and two are fast rotating (FR). Four of the BCGs show photometric signs of merging.}  \end{tabular}\\  \end{minipage}  \end{table}