Table A.1: 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.
  $\alpha$ (J2000) $\delta$ (J2000) I z
1 00:44:58.244 -29:21:10.20 18.70 0.2595
2 00:44:49.194 -29:22:12.77 17.23 0.2563
3 00:45:00.653 -29:21:43.71 19.45 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 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 0.2566
8 00:45:05.298 -29:23:10.38 18.55 0.2614
9 00:44:55.146 -29:23:18.70 18.42 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 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 0.2578
18 00:45:18.963 -29:23:53.73 16.38 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 0.2546
21 00:45:14.003 -29:23:23.38 19.85 0.2551:
22 00:45:09.830 -29:23:17.61 19.33 0.2573
23 00:45:28.259 -29:23:44.88 18.07 0.2529
24 00:45:11.115 -29:23:42.82 19.46 0.2542
25 00:45:34.024 -29:23:50.47 19.58 0.2585
26 00:45:21.197 -29:24:22.31 17.74 0.2529
27 00:45:31.420 -29:24:25.58 18.18 0.2588
28 00:45:17.220 -29:24:12.70 18.27 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 0.2600
31 00:45:30.980 -29:24:33.30 19.36 0.2531:
32 00:45:36.724 -29:24:54.63 17.24 0.2585e
33 00:45:28.202 -29:24:43.30 18.45 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 0.2585
38 00:45:25.414 -29:21:06.27 17.71 0.2537e


Source LaTeX | All tables | In the text