\begin{table}%t3 %\centering \par \caption{\label{tab_best_fit}Model parameters inferred from the lensing analysis.} $$ \begin{tabular}[c]{lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}ll} \hline\hline \noalign{\smallskip} Component & \multicolumn{2}{c}{Mass scale} & \multicolumn{2}{c}{$\theta_{1,0}$} & \multicolumn{2}{c}{$\theta_{2,0}$}& \multicolumn{2}{c}{$\epsilon$}&\multicolumn{2}{c}{$\theta_\epsilon$} & \multicolumn{2}{c}{length scale}&\multicolumn{2}{c}{} & $\log E$\\ \noalign{\smallskip} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{($\arcsec$)} &\multicolumn{2}{c}{($\arcsec$)} & \multicolumn{2}{c}{} & \multicolumn{2}{c}{($\deg$) }&\multicolumn{2}{c}{($\arcsec$)}&\multicolumn{2}{c}{}&\\ \hline \bf{All} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}& \\ \noalign{\smallskip} NFW & $0.213$&$0.017$& $1.50$&$0.17$ & $-$0.5&$0.2$ & $0.50$&$0.03$ & $-$38.3&$0.4$ & $210$&$30$& \multicolumn{2}{c}{--}&--12.4\\ \noalign{\smallskip} \hline \bf{Halo with ICM} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&\\ \noalign{\smallskip} NFW & $0.195$&$0.017$& $1.0$&$0.3$ & $-$0.6 &$0.3$ & $0.54$&$0.03$ & $-$37.2&$0.6$ & $240$&$40$ & \multicolumn{2}{c}{--}&--9.2\\ \noalign{\smallskip} \bf{All galaxies} & \multicolumn{2}{c}{$\sigma_{\rm DM}~({\rm km}~{\rm s}^{-1})$} & \multicolumn{8}{c}{}&\multicolumn{2}{c}{$r_{\rm cP}~({\rm kpc})$}&\multicolumn{2}{c}{$r_{\rm tP}~({\rm kpc})$}&\\ \noalign{\smallskip} pJaffe-$L^*$ & $85$&$19$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} & \multicolumn{2}{c}{$[45]$}&\\ \noalign{\smallskip} \hline \bf{Halo with ICM and BCG} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&\\ \noalign{\smallskip} NFW & $0.205$&$0.016$& $1.1$&$0.3$ & $-0.3$&$0.3$ & $0.52$&$0.03$ & $-37.1$&$0.7$ & $220$&$30$ & \multicolumn{2}{c}{--}&--7.6\\ \noalign{\smallskip} \bf{Other galaxies} & \multicolumn{2}{c}{$\sigma_{\rm DM}~({\rm km}~{\rm s}^{-1})$} & \multicolumn{8}{c}{}&\multicolumn{2}{c}{$r_{\rm cP}~({\rm kpc})$}&\multicolumn{2}{c}{$r_{\rm tP}~({\rm kpc})$}&\\ \noalign{\smallskip} pJaffe-$L^*$ & $90$&$20$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} & \multicolumn{2}{c}{$[45]$}&\\ \noalign{\smallskip} \hline \bf{Halo with all galaxies} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&\\ NFW & $0.206$&$0.016$& $1.47$&$0.17$ & $-0.48$&$0.19$ & $0.51$&$0.03$ & $-$40.6&$0.6$ & $170$&$20$ & \multicolumn{2}{c}{--}&--4.0\\ \noalign{\smallskip} \bf{ICM}& \multicolumn{2}{c}{$\kappa_0$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm cP}$}&\multicolumn{2}{c}{$\beta$}\\ \noalign{\smallskip} Main Clump & $0.094$&$0.011$& \multicolumn{2}{c}{[3.7]} & \multicolumn{2}{c}{[8.7]} & \multicolumn{2}{c}{[0.39]} & \multicolumn{2}{c}{[--13]} & \multicolumn{2}{c}{[13.6]} & \multicolumn{2}{c}{[0.389]}& \\ \noalign{\smallskip} Southern Tail & \multicolumn{2}{c}{[0.033]} & \multicolumn{2}{c}{[--23.4]} & \multicolumn{2}{c}{[--37.6]} & \multicolumn{2}{c}{[0.50]} & \multicolumn{2}{c}{[--37]} & \multicolumn{2}{c}{[170]} & \multicolumn{2}{c}{[1.8]}&\\ \noalign{\smallskip} \hline \bf{Halo} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&\\ \noalign{\smallskip} NFW & $0.190$&$0.019$& $1.2$&$0.5$ & $-0.4$&$0.3$ & $0.53$&$0.03$ & $-40$&$1$ & $190$&$30$ & \multicolumn{2}{c}{--}&--1.9\\ \noalign{\smallskip} \bf{All galaxies} & \multicolumn{2}{c}{$\sigma_{\rm DM}~({\rm km}~{\rm s}^{-1})$} & \multicolumn{8}{c}{}&\multicolumn{2}{c}{$r_{\rm cP}~({\rm kpc})$}&\multicolumn{2}{c}{$r_{\rm tP}~({\rm kpc})$}&\\ \noalign{\smallskip} pJaffe-$L^*$ & $70$&$30$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} & \multicolumn{2}{c}{$[45]$}&\\ \noalign{\smallskip} \bf{ICM}& \multicolumn{2}{c}{$\kappa_0$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm cP}$}&\multicolumn{2}{c}{$\beta$}\\ \noalign{\smallskip} Main Clump & $0.093$&$0.013$& \multicolumn{2}{c}{[3.7]} & \multicolumn{2}{c}{[8.7]} & \multicolumn{2}{c}{[0.39]} & \multicolumn{2}{c}{[--13]} & \multicolumn{2}{c}{[13.6]} & \multicolumn{2}{c}{[0.389]}& \\ \noalign{\smallskip} Southern Tail & \multicolumn{2}{c}{[0.033]} & \multicolumn{2}{c}{[--23.4]} & \multicolumn{2}{c}{[--37.6]} & \multicolumn{2}{c}{[0.50]} & \multicolumn{2}{c}{[--37]} & \multicolumn{2}{c}{[170]} & \multicolumn{2}{c}{[1.8]}&\\ \noalign{\smallskip} \hline \bf{Halo with BCG} & \multicolumn{2}{c}{$\kappa_{\rm NFW}$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&\\ \noalign{\smallskip} NFW & $0.198$&$0.017$& $1.2$&$0.3$ & $-0.3$&$0.3$ & $0.53$&$0.03$ & $-39.4$&$0.9$ & $180$&$30$ & \multicolumn{2}{c}{--}&0.0\\ \noalign{\smallskip} \bf{Other galaxies} & \multicolumn{2}{c}{$\sigma_{\rm DM}~({\rm km}~{\rm s}^{-1})$} & \multicolumn{8}{c}{}&\multicolumn{2}{c}{$r_{\rm cP}~({\rm kpc})$}&\multicolumn{2}{c}{$r_{\rm tP}~({\rm kpc})$}&\\ \noalign{\smallskip} pJaffe & $80$&$20$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} & \multicolumn{2}{c}{$[45]$}&\\ \noalign{\smallskip} \bf{ICM}& \multicolumn{2}{c}{$\kappa_0$} & \multicolumn{8}{c}{} &\multicolumn{2}{c}{$r_{\rm cP}$}&\multicolumn{2}{c}{$\beta$}\\ \noalign{\smallskip} Main Clump & $0.092$&$0.013$& \multicolumn{2}{c}{[3.7]} & \multicolumn{2}{c}{[8.7]} & \multicolumn{2}{c}{[0.39]} & \multicolumn{2}{c}{[--13]} & \multicolumn{2}{c}{[13.6]} & \multicolumn{2}{c}{[1.833]}& \\ \noalign{\smallskip} Southern Tail & \multicolumn{2}{c}{[0.033]} & \multicolumn{2}{c}{[--23.4]} & \multicolumn{2}{c}{[--37.6]} & \multicolumn{2}{c}{[0.50]} & \multicolumn{2}{c}{[--37]} & \multicolumn{2}{c}{[170]} & \multicolumn{2}{c}{[--2.4]}&\\ \noalign{\smallskip} \hline \end{tabular} $$ \tablefoot{For each model, the first line specifies the mass components accounted by the cluster-sized halo, parameterized as a NFW distribution.``All'' refers to a mass model (DM+baryons) with a single NFW component. The other models may have additional components either for the gas or the galactic halos. The BCG is either scaled as the other galaxies (``All galaxies'') or embedded in the cluster-zised halo (halos ``with BCG''). The ICM is either modelled apart or embedded in the cluster-sized halo (``Halo with ICM''). The orientation angle $\theta_\epsilon$ is measured north over east and $r_{\rm sP}$ ($r_{\rm cP}$) is the projected length scale (core radius) for the NFW ($\beta$) profile. Parameters in squared brackets were kept fixed in the lensing analysis. Convergences are normalised to the E system source redshift.} \end{table}