\begin{table*}%[!]%t3
\begin{table}
%\setlength{\tabcolsep}{4.5pt}
\caption{Summary of the main properties of SL2S groups.}
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\begin{tabular}{lcccccccccccccc}
\hline\hline
SL2S Group & RA & Dec & $z_{\rm spec}$ & $z_{\rm phot}$ & $R_{\textsc{e}}$ (\textsc{sl}) & $R_{\textsc{e}}$ (\textsc{wl}) & $D_{\rm ls}$/$D_{\rm s}$ & $z_{\rm eff}$ & $\sigma_{\rm SIS}$ (\textsc{wl}) & $M_{\textsc{wl}}$\,(2\,Mpc) & $N_{\rm bckg}$ & $L$ & Seeing & $M_{\rm c}$ \\
\hline
J09013-0158 &  135.41443 &  --1.9811666 & -- & $\rm 0.296^{+0.052}_{-0.017}$ &$\sim$6.8 & $3.83\pm2.97$ & 0.487 & 0.641 & $\rm 521^{+174}_{-274}$ & $4.0\pm3.1$ $(3.9\pm3.0)$ & 11.8 & $2.78\pm0.38$ & 0.80 &24.13 \\
J22214-0053 & 335.43226 & --0.88404303 &  0.334  & $\rm 0.314^{+0.026}_{-0.057}$ & $6.83\pm0.15$ & $3.15\pm3.10$ & 0.448  & 0.660 & $\rm 494^{+201}_{-432}$ & $3.6\pm3.5$ $(3.5\pm3.4)$ & 10.3 & $1.36\pm0.27$ & 0.72  &  24.60 \\
J08544-0121 & 133.69395 &  --1.3603506 & 0.351 & $\rm 0.324^{+0.067}_{-0.013}$ & $5.48\pm0.12$ &  $5.37\pm2.12$ & 0.430 & 0.671 & $\rm 658^{+119}_{-146}$ & $6.3\pm2.5$ $(6.2\pm2.4)$ & 13.5 & $3.29\pm0.40$ & 0.51 & 23.91\\
J09413-1100 & 145.39478 & --11.015091 & 0.385 &  $\rm 0.418^{+0.007}_{-0.005}$ &$7.50\pm0.81$ &  $2.98\pm2.64$ & 0.393 & 0.688 & $\rm 508^{+189}_{-337}$  & $3.7\pm3.4$ $(3.7\pm3.3)$ & 10.4 & $1.27\pm0.24$ & 0.69 & 24.25 \\
J14081+5429 & 212.05808 & 54.484634 & 0.416 &  $\rm 0.436^{+0.016}_{-0.039}$ & $\sim$4.5 & $<$4.83 & 0.362 & 0.705 & $<$680 & $<$6.8 (6.6) & 10.8  & $2.46\pm0.39$ & 0.72 & 23.61 \\
J14300+5546 & 217.50275 & 55.779964  & 0.435 &  $\rm 0.486^{+0.028}_{-0.024}$ &$4.69\pm1.43$ & 
$<$4.64 & 0.344 & 0.715 & $<$684 & $<$6.8 (6.6) & 14.7 & $2.15\pm0.27$ & 0.72 & 24.39 \\
J02140-0532& 33.533465 & --5.5923947  & 0.444 & $\rm 0.440^{+0.026}_{-0.016}$ & $7.31\pm0.49$ & $3.62\pm2.45$& 0.335 & 0.719 & $\rm 612^{+180}_{-264}$ & $5.5\pm3.7$ $(5.3\pm3.6)$ & 13.0 &  $2.90\pm0.39$ & 0.61 & 23.96 \\
J02254-0737 & 36.44216 & --7.6273523 & 0.511 & $\rm 0.480^{+0.016}_{-0.016}$ & $6.00\pm0.31$ & 
$<$2.56 & 0.274 & 0.751 & $<$569 & $<$4.7 (4.4) & 11.9  & $1.93\pm0.30$ & 0.67 & 23.76  \\
J22130-0030 & 333.27883 & --0.51030426 & -- & $\rm 0.606^{+0.012}_{-0.029}$ & $\sim$3.6 & $<$3.06 & 0.201 & 0.805 & $<$726 & $<$6.9 (6.2) & 11.8 & $3.19\pm0.50$ & 0.61 & 24.41 \\
J02215-0647 & 35.463263 & -6.792443 &  0.618 & $\rm 0.636^{+0.028}_{-0.044}$ & $2.56\pm0.14$  & 
$<$1.22 & 0.196 & 0.810 & $<$463 & $<$3.1 (2.8) & 12.0 & $1.50\pm0.27$ & 0.51 & 24.24 \\
J14314+5533 & 217.9156 & 55.556308 & -- & $\rm 0.640^{+0.143}_{-0.069}$ & $\sim$2.5 & $<$3.98 & 0.182 &0.822 & $<$870 & $<$11.1 (9.9) & 13.4 & $3.55\pm0.48$ & 0.72 & 24.14 \\
J08591-0345 & 134.81024 &  --3.7540217 &  0.647 & $\rm 0.586^{+0.040}_{-0.016}$ & $\sim$ 8 & -- & -- & -- & --  & -- & -- &--& 0.82 & 23.79 \\
J22133+0048 & 333.38274 &  0.81002713 & -- & $\rm 0.826^{+0.022}_{-0.032}$ & $3.40\pm0.2$  & $2.46\pm1.91$ & 0.095 & 0.946 & $\rm 947^{+315}_{-499}$ & $13.1\pm10.2$ $(10.8\pm8.5)$ & 11.1 &  $3.34\pm0.54$ & 0.54 & 24.08 \\
\hline
\end{tabular}
\smallskip
 {J\,2000.0 coordinates of the main galaxy populating the deflector;
spectroscopic redshift $z_{\rm spec}$; photometric redshift $z_{\rm phot}$; Einstein radius derived from the strong lensing modelling, when possible.
For the non cusp group, we report with a \~\ the distance between the lensed feature and the brighest
group member;
Einstein radius derived from fitting a Singular Isothermal Sphere (SIS) to the weak lensing signal;
mean geometrical factor $D_{\rm ls}$/$D_{\rm s}$ and corresponding effective redshift~$z_{\rm eff}$; velocity dispersion;
projected mass derived from weak lensing computed within a circular aperture of radius equals to 2\,Mpc, in units 10$^{14}$~$M_{\odot}$
(masses derived using the \citet{coupon} photometric redshift catalogue are given within brackets);
density of background galaxies, expressed in objects per square arcminute;
total $i$~band rest frame luminosity corrected for evolution, in units 10$^{12}$~$L_{\odot}$;
seeing of the $i$~band observations; $i$~band completeness magnitude.
Einstein radii and seeings are expressed in arcseconds.}  \label{res}
\end{table}