A multiwavelength strong lensing analysis of baryons and dark matter in the dynamically active cluster AC 114

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Table 4:

Model parameters inferred from the lensing analysis when the cluster-sized halo is modelled as a NIE and $r_{\rm cP}$ is the projected core radius.
$\begin{displaymath}\begin{tabular}[c]{lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~... ...{c}{[170]} & \multicolumn{2}{c}{[1.8]}&\\ \hline \end{tabular}\end{displaymath}$ Notes. The BCG is scaled either in the same way as the other galaxies or varied independently (see models with a ``pJaffe-BCG'' component). The ICM is either modelled apart (``Halo'') or embedded in the cluster-sized halo (``Halo with ICM'').

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