All Tables

Table 1: Left: relative positions between the different lensed components (B, C, D) and the lensing galaxy (G) with respect to component A as deducted from the best seeing EFOSC-2 frame using the GENERAL (GEN) and MCS codes (see text). Right: relative magnitude of the B, C, D lensed images with respect to A deducted with the MCS method at two different epochs. The last two columns give respectively the amplification $\mu_{\textrm{\tiny{exp}}}$ (sign = parity) predicted by the SIS $+\gamma$ model and the corresponding relative magnitude with respect to A (Sect. 4).