deletions | additions       diff --git a/section_Previous_measurements_citet_JIMMY13__.tex b/section_Previous_measurements_citet_JIMMY13__.tex  index 0f57194..a617b22 100644  --- a/section_Previous_measurements_citet_JIMMY13__.tex  +++ b/section_Previous_measurements_citet_JIMMY13__.tex 
...
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}.  \texbf{Kinematic \\\textbf{Kinematic  properties of BCGs and their companions from \citet{JIMMY13}. \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.} 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 \\   & &$\pm0.01$ &$\pm 0.01$ &$G-M_{20}$} & &$G-M_{20}$&  \\ \hline\hline BCGs&&&&&\\  1027A& 0.090 &11.79& 6.98 & y &SR\\  1042& 0.094 &11.83& 7.22 & n & SR\\