\begin{table}%t
%\centering
\par
\caption{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{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}{}&\\
        \noalign{\smallskip}
        \hline
        \noalign{\smallskip}
\bf{Halo with ICM} & \multicolumn{2}{c}{$b~(\arcsec)$} & \multicolumn{8}{c}{}
&\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&--13.7\\
        \noalign{\smallskip}
        NIE & $27$&$2$& $0.2$&$0.7$ & $-$0.4&$0.7$ & $0.59$&$0.04$ & $-$35.2&$0.6$
& $11.9$&$1.4$ & \multicolumn{2}{c}{-}&\\
        \noalign{\smallskip}
        \bf{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^*$ & $147$&$13$ & \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} & \multicolumn{2}{c}{$b~(\arcsec)$} & \multicolumn{8}{c}{}
&\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&--6.7\\
        \noalign{\smallskip}
        NIE & $31$&$3$& $0.8$&$0.8$ & $-0.6$&$0.7$ & $0.55$&$0.04$ & $-36.4$&$0.6$
& $13.7$&$1.4$ & \multicolumn{2}{c}{--}&\\
        \noalign{\smallskip}
        \bf{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^*$ & $110$&$20$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} &
\multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} &
\multicolumn{2}{c}{$[45]$}&\\
pJaffe-BCG & $239$&$18$ & \multicolumn{2}{c}{[0.0]} & \multicolumn{2}{c}{[0.0]} &
\multicolumn{2}{c}{[0.42]} & \multicolumn{2}{c}{[-32.8]} & \multicolumn{2}{c}{$[0.29]$} &
\multicolumn{2}{c}{$[87]$}&\\
\noalign{\smallskip}
\hline
\bf{Halo} & \multicolumn{2}{c}{$b~(\arcsec)$} & \multicolumn{8}{c}{}
&\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&--5.9\\
        \noalign{\smallskip}
        NIE & $23.3$&$1.3$& $0.4$&$0.6$ & $-$0.1 &$0.6$ & $0.57$&$0.04$ & $-$37.3 &$0.8$
& $11.1$&$1.2$ & \multicolumn{2}{c}{--}&\\
        \noalign{\smallskip}
        \bf{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^*$ & $137$&$12$ & \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 & $0.091$&$0.015$&  \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}{$b~(\arcsec)$} & \multicolumn{8}{c}{}
&\multicolumn{2}{c}{$r_{\rm sP}$}&\multicolumn{2}{c}{}&3.2\\
        \noalign{\smallskip}
        NIE & $26$&$2$& $1.1$&$0.8$ & $-$0.3 &$0.7$ & $0.53$&$0.04$ & $-$39.0 &$1.1$& $12.9$&$1.0$ & \multicolumn{2}{c}{-}&\\
        \noalign{\smallskip}
        \bf{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^*$ & $140$&$40$ & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} &
\multicolumn{2}{c}{--} & \multicolumn{2}{c}{--} & \multicolumn{2}{c}{$[0.15]$} &
\multicolumn{2}{c}{$[45]$}&\\
pJaffe-BCG & $227$&$18$& \multicolumn{2}{c}{[0.0]} & \multicolumn{2}{c}{[0.0]} &
\multicolumn{2}{c}{[0.42]} & \multicolumn{2}{c}{[--32.8]} & \multicolumn{2}{c}{$[0.29]$} &
\multicolumn{2}{c}{$[87]$}&\\
\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$&$0.012$&  \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]}&\\ 
\hline
\end{tabular}
$$
\tablefoot{\label{tab_best_is}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'').}
\end{table}