Table 5: Heliocentric redshifts for CL0056.03, taken from CHM98. Here, v denotes the radial velocity in $\rm{km~s^{-1}}$ together with its measurement errors $\sigma _v$, and the index m indicates whether a galaxy is closer to the eastern cD galaxy ( ${\rm ID}=6$), or to the western one ( ${\rm ID}=16$).

ID		 RA (2000.0) DEC (2000.0) v $\sigma_{\rm v}$ z m

1		 00:56:10.23 -37:34:07.9 51570 282 0.17202 1
2 00:56:09.22 -37:33:59.5 50799 51 0.16945 1
3 00:56:07.07 -37:33:49.4 51628 138 0.17221 1
4 00:56:09.71 -37:33:39.9 50709 120 0.16915 1
5 00:56:01.49 -37:33:31.6 49315 111 0.16450 1
6 00:56:06.41 -37:33:18.0 49754 154 0.16596 cD 1
7 00:55:57.50 -37:32:51.5 46839 38 0.15624 2
8 00:55:58.90 -37:33:00.7 48490 50 0.16175 2
9 00:56:02.76 -37:33:03.9 49588 192 0.16541 1
10 00:56:04.76 -37:33:00.3 50394 117 0.16810 1
11 00:56:04.75 -37:32:51.0 51594 84 0.17210 1
12 00:55:55.59 -37:32:20.2 48514 145 0.16183 2
13 00:55:56.74 -37:32:35.4 49555 123 0.16530 2
14 00:55:57.74 -37:32:23.4 48256 101 0.16096 2
15 00:55:59.32 -37:32:35.2 49041 145 0.16358 2
16 00:55:59.09 -37:32:18.2 48888 117 0.16307 cD 2
17 00:56:01.32 -37:32:41.9 50168 187 0.16734 2
18 00:56:02.45 -37:32:18.0 47381 138 0.15805 2
19 00:56:02.41 -37:32:05.7 49097 113 0.16377 2
20 00:55:56.18 -37:31:48.3 49439 14 0.16491 2
21 00:56:09.54 -37:31:49.0 49863 107 0.16633 1


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