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Table A.1

Sample S1 of the background group at z ~ 0.1.

RA Dec z Sample

23:12:13.8 42:46:36 0.1067 S1
23:12:17.8 42:47:10 0.1065 S1
23:12:41.7 42:28:04 0.1166 S1
23:12:46.5 42:56:27 0.1134 S1
23:12:51.7 42:31:05 0.1000 S2
23:12:54.0 42:30:50 0.0997 S2
23:13:04.7 42:52:59 0.1002 S2
23:13:12.0 42:29:34 0.1002 S2
23:13:13.6 42:27:31 0.0914 S1
23:13:14.3 42:29:59 0.1012 S2
23:13:14.5 42:29:57 0.1003 S2
23:13:24.0 42:53:05 0.1167 S1
23:13:25.9 42:58:08 0.0922 S1
23:13:27.5 42:32:05 0.0983 S2
23:13:33.6 42:27:33 0.1001 S2
23:13:39.1 42:48:23 0.1164 S1
23:13:41.2 42:42:03 0.1160 S1
23:13:41.5 42:32:42 0.0992 S2
23:13:41.8 42:34:15 0.0993 S2
23:13:43.4 42:28:00 0.0994 S2
23:13:46.2 42:30:35 0.1056 S1
23:13:46.9 42:34:38 0.0995 S2
23:13:48.4 42:31:24 0.1065 S1
23:13:49.5 42:26:34 0.0993 S2
23:13:50.8 42:30:00 0.1055 S1
23:13:52.7 42:28:47 0.1003 S2
23:13:52.8 42:28:23 0.1006 S2
23:13:52.8 42:28:25 0.1062 S1
23:13:54.4 42:29:21 0.1009 S2
23:13:55.4 42:26:19 0.0996 S2
23:13:55.8 42:29:51 0.0993 S2
23:13:56.8 42:39:02 0.1044 S1
23:13:57.2 42:59:11 0.1149 S1
23:13:57.6 42:31:44 0.0986 S2
23:13:57.9 42:33:02 0.0985 S2
23:14:03.3 42:29:13 0.0992 S2
23:14:07.7 42:41:17 0.0998 S2
23:14:09.6 42:27:04 0.1005 S2
23:14:09.7 42:33:33 0.0996 S2
23:14:13.1 42:32:23 0.0995 S2
23:14:14.3 42:46:33 0.1156 S1
23:14:20.5 42:36:21 0.1057 S1
23:14:22.7 42:38:03 0.1051 S1
23:14:25.7 42:37:28 0.1039 S1
23:14:28.1 42:40:16 0.1163 S1
23:14:30.9 42:42:17 0.1166 S1
23:14:33.3 42:39:47 0.0994 S2
23:14:50.7 42:20:06 0.0914 S1
23:14:59.8 42:33:44 0.1156 S1
23:15:06.7 42:35:18 0.1157 S1
23:15:11.5 42:34:52 0.1158 S1
23:15:22.2 42:34:03 0.1005 S1
23:15:52.2 42:25:47 0.1029 S2

Notes. The subsample S2 is included in S1 but is highlighted for simplicity only as a subgroup (see Col. 4). While S1 corresponds to a simple velocity-clipped sample, S2 is based on biweight estimates and iterative sigma-clipping (see Sect. 6 for details). Galaxies of the latter sample are considered group members of LCLG −42 230. Position in RA and Dec (J2000) is based on GSC2.3 astrometry. The spectroscopic redshift is given in Col. 3.

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