Table 3: Best values of the Sérsic and de Vaucouleurs (dVc) profiles fitted to the lensing galaxy (see Sect. 4.3 for details). Quoted errors are the 1$\sigma $ dispersion of the results on the NExp individual frames. The number of d.o.f. is about 3120 for F555W and F814W frames, and about 1100 for F160 frames.

Filter		 Model $\mu_{\rm e}(z)$ (mag/arcsec2) $q_{\rm s}$ $\varphi$(PA) $R_{\rm e}$ (kpc h-150) n $\chi^2$/d.o.f.

F555W		 Sérsic $21.84\pm0.38$ $0.96\pm0.01$ $-22^\circ\pm20$ $4.69\pm0.77$ $2.19\pm 0.22$ 2.53
  dVc $23.35\pm0.21$ $0.96\pm0.02$ $-60^\circ\pm32$ $10.48\pm0.88$ 4 2.76
F814W Sérsic $20.36\pm0.17$ $0.94\pm0.01$ $-56^\circ.1\pm2.6$ $5.05\pm0.37$ $2.67\pm 0.12$ 3.62
  dVc $21.49\pm0.05$ $0.93\pm0.01$ $-64^\circ.2\pm1.9$ $9.33\pm0.18$ 4 3.98
F160W Sérsic $18.09\pm0.22$ $0.92\pm0.01$ $-62^\circ.2\pm4.1$ $4.16\pm0.41$ $2.71\pm 0.16$ 18.8
  dVc $19.28\pm0.14$ $0.91\pm0.01$ $-65^\circ.3\pm3.8$ $8.33\pm0.51$ 4 19.9

Source LaTeX | All tables | In the text