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Table 3:

Summary of the main properties of SL2S groups.
SL2S Group RA Dec $z_{\rm spec}$ $z_{\rm phot}$ $R_{\textsc{e}}$ (SL) $R_{\textsc{e}}$ (WL) $D_{\rm ls}$/$D_{\rm s}$ $z_{\rm eff}$ $\sigma_{\rm SIS}$ (WL) $M_{\textsc{wl}}$(2Mpc) $N_{\rm bckg}$ L Seeing $M_{\rm c}$
J09013-0158 135.41443 -1.9811666 - $\rm0.296^{+0.052}_{-0.017}$ $\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 $\rm0.314^{+0.026}_{-0.057}$ $6.83\pm0.15$ $3.15\pm3.10$ 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 $\rm0.324^{+0.067}_{-0.013}$ $5.48\pm0.12$ $5.37\pm2.12$ 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 $\rm0.418^{+0.007}_{-0.005}$ $7.50\pm0.81$ $2.98\pm2.64$ 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 $\rm0.436^{+0.016}_{-0.039}$ $\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 $\rm0.486^{+0.028}_{-0.024}$ $4.69\pm1.43$ <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 $\rm0.440^{+0.026}_{-0.016}$ $7.31\pm0.49$ $3.62\pm2.45$ 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 $\rm0.480^{+0.016}_{-0.016}$ $6.00\pm0.31$ <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 - $\rm0.606^{+0.012}_{-0.029}$ $\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 $\rm0.636^{+0.028}_{-0.044}$ $2.56\pm0.14$ <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 - $\rm0.640^{+0.143}_{-0.069}$ $\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 $\rm0.586^{+0.040}_{-0.016}$ $\sim $ 8 - - - - - - - 0.82 23.79
J22133+0048 333.38274 0.81002713 - $\rm0.826^{+0.022}_{-0.032}$ $3.40\pm0.2$ $2.46\pm1.91$ 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
J2000.0 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 2Mpc, in units 1014 $M_{\odot}$(masses derived using the Coupon et al. (2008) 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 1012 $L_{\odot }$; seeing of the i band observations; i band completeness magnitude. Einstein radii and seeings are expressed in arcseconds.

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