deletions | additions       diff --git a/section_Previous_measurements_citet_JIMMY13__.tex b/section_Previous_measurements_citet_JIMMY13__.tex  index b9b0d05..d3cc259 100644  --- a/section_Previous_measurements_citet_JIMMY13__.tex  +++ b/section_Previous_measurements_citet_JIMMY13__.tex 
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G \geq -0.14M_{20} + 0.33  \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}.  \small{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}{ c c c c c c }  \label{tab:kin}  Galaxy & $z$ & log M$_{\rm dyn}$~M$_{\odot}$ & R$_e$(arcsec) & Merging & SR/FR \\   & & \tiny{$\pm0.01$} & \tiny{$\pm 0.01$} & \tiny{$G-M_{20}$} & \\   \hline\hline 
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1048B& 0.080 &10.51&1.08&y&FR\\  1048C& 0.074 &10.54&1.24&y&FR\\  \end{tabular}  \\  \small{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.}