\begin{table}%tA.1
\par
\caption{Redshifts obtained in the EISJ0045-2923 field. Here and in
the following tables an attached ":'' represents a less secure
redshift as described in the text, and an "e'' represents that the
galaxy has one or more emission lines. The galaxies with redshifts in
bold face are the ones considered members of the cluster.}
\label{tab:z_J0045-2923}
\par
%\centering
\par
\begin{tabular}{r c c c l}
\hline\hline
 & $\alpha$ (J2000) & $\delta$ (J2000) & I & \multicolumn{1}{c}{$z$} \\
\hline
  1 & 00:44:58.244 & $-$29:21:10.20 & 18.70 & {\bf 0.2595}\\
  2 & 00:44:49.194 & $-$29:22:12.77 & 17.23 & {\bf 0.2563}\\
  3 & 00:45:00.653 & $-$29:21:43.71 & 19.45 & {\bf 0.2564:}\\
  4 & 00:44:49.431 & $-$29:22:24.31 & 18.08 & 0.1787\\
  5 & 00:44:54.988 & $-$29:22:24.26 & 17.81 & {\bf 0.2566}\\
  6 & 00:44:57.079 & $-$29:22:34.95 & 18.27 & 0.1361e\\
  7 & 00:45:05.872 & $-$29:22:53.03 & 18.84 & {\bf 0.2566}\\
  8 & 00:45:05.298 & $-$29:23:10.38 & 18.55 & {\bf 0.2614}\\
  9 & 00:44:55.146 & $-$29:23:18.70 & 18.42 & {\bf 0.2575e}\\
 10 & 00:45:02.491 & $-$29:23:51.99 & 19.95 & 0.3385e\\
 11 & 00:45:15.789 & $-$29:25:28.17 & 18.76 & 0.4479\\
 12 & 00:45:06.614 & $-$29:26:11.01 & 18.58 & 0.3200e\\
 13 & 00:45:08.261 & $-$29:22:45.04 & 16.55 & 0.1828e\\
 14 & 00:45:23.627 & $-$29:22:00.88 & 18.59 & 0.1368e\\
 15 & 00:45:09.216 & $-$29:22:46.49 & 17.89 & {\bf 0.2586}\\
 16 & 00:45:26.346 & $-$29:22:18.45 & 18.27 & 0.1698\\
 17 & 00:45:16.708 & $-$29:22:45.86 & 18.28 & {\bf 0.2578}\\
 18 & 00:45:18.963 & $-$29:23:53.73 & 16.38 & {\bf 0.2572}\\
 19 & 00:45:11.432 & $-$29:23:00.03 & 18.87 & 0.4465:\\
 20 & 00:45:22.118 & $-$29:22:58.33 & 18.33 & {\bf 0.2546}\\
 21 & 00:45:14.003 & $-$29:23:23.38 & 19.85 & {\bf 0.2551:}\\
 22 & 00:45:09.830 & $-$29:23:17.61 & 19.33 & {\bf 0.2573}\\
 23 & 00:45:28.259 & $-$29:23:44.88 & 18.07 & {\bf 0.2529}\\
 24 & 00:45:11.115 & $-$29:23:42.82 & 19.46 & {\bf 0.2542}\\
 25 & 00:45:34.024 & $-$29:23:50.47 & 19.58 & {\bf 0.2585}\\
 26 & 00:45:21.197 & $-$29:24:22.31 & 17.74 & {\bf 0.2529}\\
 27 & 00:45:31.420 & $-$29:24:25.58 & 18.18 & {\bf 0.2588}\\
 28 & 00:45:17.220 & $-$29:24:12.70 & 18.27 & {\bf 0.2644}\\
 29 & 00:45:30.082 & $-$29:24:32.86 & 19.30 & 0.4804\\
 30 & 00:45:12.996 & $-$29:24:30.78 & 19.40 & {\bf 0.2600}\\
 31 & 00:45:30.980 & $-$29:24:33.30 & 19.36 & {\bf 0.2531:}\\
 32 & 00:45:36.724 & $-$29:24:54.63 & 17.24 & {\bf 0.2585e}\\
 33 & 00:45:28.202 & $-$29:24:43.30 & 18.45 & {\bf 0.2530}\\
 34 & 00:45:37.375 & $-$29:24:43.14 & 19.52 & 0.3306\\
 35 & 00:45:35.645 & $-$29:25:54.91 & 18.56 & 0.3550\\
 36 & 00:45:39.744 & $-$29:25:46.61 & 18.17 & 0.3232e\\
 37 & 00:45:32.465 & $-$29:25:46.35 & 18.55 & {\bf 0.2585}\\
 38 & 00:45:25.414 & $-$29:21:06.27 & 17.71 & {\bf 0.2537e}\\
\hline
\end{tabular}
\end{table}