\begin{table}%t3 
\caption{\label{newmul} Location and redshift estimate of three new multiply-image systems, as well as the radial feature~(10.4) associated with the giant arc (systems~10 and~11).}
%\centerline
 {\begin{tabular}{lcclllr}
\hline\hline
ID & $\alpha$ (J2000.0) & $\delta$ (J2000.0) & $z_{\rm model}$ & $z_{\rm phot}$ & $F775W$ & $\mu$ (mags)\\
\hline 
\multicolumn{3}{l}{New multiple images} \\
10.4 & 198.77173 & 51.81906 & $z_{\rm spec}=2.627$ & $-$ & $24.77\pm0.08$ & $1.55\pm0.17$ \\
12.1 & 198.77456 & 51.829946 & {$3.31\pm0.16$} & $\rm 3.33^{+0.47}_{-0.32}$ & $26.68\pm0.10$ & $1.93\pm0.07$\\
12.2 & 198.76568 & 51.828658 & & $\rm 3.35^{+0.22}_{-0.31}$                                    & $24.47\pm0.04$ & $1.87\pm0.16$ \\
12.3 & 198.75867 & 51.826482 & & $\rm 3.16^{+0.24}_{-0.52}$                                    & $26.33\pm0.08$ & $2.17\pm0.04$ \\
13.1 & 198.78238 & 51.821204 & {$0.839\pm0.007$} & $\rm 1.15^{+0.13}_{-0.16}$ & $26.93\pm0.11$& $1.48\pm0.03$\\
13.2 & 198.76796 & 51.818374 & & $\rm 0.68^{+0.46}_{-0.12}$                                    & $24.18\pm0.04$ & $2.42\pm0.33$\\
13.3 & 198.77204 & 51.814973 & & $\rm 1.13^{+0.08}_{-0.10}$                                    & $26.29\pm0.08$ & $2.16\pm0.19$\\
13.4 & 198.76692 & 51.815130 & & $\rm 1.07^{+0.19}_{-0.10}$                                    & $25.12\pm0.05$ & $2.69\pm0.06$\\
14.1 & 198.78662 & 51.820542 & {$1.58\pm0.02$} & $-$                                         & $25.55\pm0.11$ & $1.63\pm0.02$\\
14.2 & 198.76868 & 51.820191 & & $-$                                                                        & $25.40\pm0.17$ & $1.26\pm0.48$\\
14.3 & 198.76447 & 51.812192 & & $-$                                                                        & $26.33\pm0.16$ & $2.13\pm0.03$\\
14.4 & 198.77540 & 51.811945 & & $-$                                                                        & $26.30\pm0.15$ & $0.81\pm0.10$\\
\hline
\multicolumn{3}{l}{Other multiple systems from L08}\\
2.2 & 198.77156 & 51.81174 & $\rm 2.16^{+0.15}_{?0.09}$ & $\rm 2.31^{+0.46}_{-0.38}$ & $25.29\pm0.08$ & $4.45\pm0.18$\\
2.3 & 198.76970 & 51.81186 &  & $\rm 2.23^{+0.19}_{-0.66}$ & $26.15\pm0.10$ & $4.37\pm0.16$\\
8.1 & 198.77250 & 51.83045 & $\rm 2.933^{+0.004}_{-0.077}$  & $\rm 2.80^{+0.17}_{-0.09}$ & $24.95\pm0.06$ & $2.46\pm0.18$\\ 
8.2 & 198.76608 & 51.82949 & & $\rm 2.77^{+0.21}_{-0.11}$ & $23.06\pm0.02$ & $2.19\pm0.10$\\
8.3 & 198.75863 & 51.82740 & & $\rm 2.72^{+0.20}_{-0.12}$ & $25.07\pm0.06$ & $2.00\pm0.03$\\ 
9.1 & 198.77176 & 51.83030 & $\rm 3.271^{+0.031}_{-0.124}$ & $-$ & $26.68\pm0.15$ & $3.09\pm0.20$\\
9.2 & 198.76690 & 51.82957 & & $\rm 2.995^{+0.195}_{-0.378}$ & $25.32\pm0.08$ & $2.48\pm0.19$\\
9.3 & 198.75813 & 51.82708 & & $\rm 3.00^{+0.37}_{-0.60}$ & $26.92\pm0.12$ & $1.98\pm0.02$\\
\hline
\end{tabular}}
\medskip 
From left to right: identification, astrometric position, redshift estimate from the lensing model, photometric redshift estimate, magnification in magnitudes.  We also report the same values for the three remaining systems from L08 (systems~2, 8~and~9), used in the mass model but lacking spectroscopic redshifts. The redshift of 10.4 has a spectroscopic measurement and therefore is not a free parameter in the model. System~14 and image~9.1 are too faint to provide a reliable photometric redshift estimate.
\end{table}