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Paola Oliva-Altamirano edited section_Previous_measurements_citet_JIMMY13__.tex
almost 9 years ago
Commit id: e9093a71d0f102f0d2afd39ac11784e95ddbfdae
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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}.
\begin{tabular}{ c c c c c c }
Galaxy & $z$ & log M$_{\rm dyn}$~M$_{\odot}$ & R$_e$(arcsec) & Merging & SR/FR \\
& & \tiny{$\pm0.01$} & \tiny{$\pm 0.01$} & \tiny{$G-M_{20}$} & \\
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\end{tabular}
\begin{tabular}{lccccc}