Table B.1
Sample of spectroscopically confirmed cluster members of S1101.
| RA | Dec | z | Type | R | Reference |
|
|
|||||
| 23:11:40.7 | −43:06:31 | 0.05694 | 0 | – | Jones et al. (2009) |
| 23:11:47.7 | −43:05:21 | 0.05571 | 1 | – | Jones et al. (2009) |
| 23:12:03.2 | −42:54:13 | 0.05532 | 1 | 15.860 | – |
| 23:12:15.2 | −42:44:28 | 0.05349 | 0 | 17.611 | – |
| 23:12:19.9 | −42:53:50 | 0.05800 | 0 | 15.518 | Jones et al. (2009) |
| 23:12:40.5 | −42:53:16 | 0.05602 | 0 | 16.208 | – |
| 23:12:41.0 | −42:54:28 | 0.05595 | 1 | 18.487 | – |
| 23:12:53.1 | −42:29:19 | 0.05589 | 1 | 18.837 | – |
| 23:13:02.2 | −42:36:36 | 0.05589 | 0 | 15.272 | – |
| 23:13:06.0 | −42:33:21 | 0.05721 | 0 | 18.481 | – |
| 23:13:12.2 | −42:24:36 | 0.05562 | 99 | – | Shectman et al. (1996) |
| 23:13:13.3 | −42:41:07 | 0.05495 | 0 | 15.013 | – |
| 23:13:13.5 | −42:27:27 | 0.05626 | 0 | 16.360 | – |
| 23:13:16.0 | −42:38:11 | 0.05673 | 0 | 16.195 | – |
| 23:13:17.4 | −42:22:22 | 0.05556 | 99 | – | Shectman et al. (1996) |
| 23:13:25.5 | −42:30:32 | 0.05432 | 1 | 16.204 | – |
| 23:13:29.7 | −42:28:27 | 0.05792 | 0 | 15.819 | Jones et al. (2009) |
| 23:13:34.6 | −42:38:17 | 0.05421 | 0 | 18.938 | – |
| 23:13:37.5 | −42:39:42 | 0.05716 | 0 | 20.064 | – |
| 23:13:38.9 | −43:01:09 | 0.05934 | 0 | 17.177 | – |
| 23:13:41.4 | −42:35:20 | 0.05424 | 0 | 19.584 | – |
| 23:13:46.0 | −42:45:22 | 0.05165 | 0 | 17.429 | – |
| 23:13:48.8 | −42:46:34 | 0.05246 | 0 | 15.274 | – |
| 23:13:48.9 | −42:47:09 | 0.05404 | 0 | 15.822 | – |
| 23:13:49.6 | −42:44:44 | 0.05583 | 0 | 17.653 | – |
| 23:13:50.9 | −42:45:46 | 0.05719 | 0 | 16.504 | – |
| 23:13:52.3 | −42:42:39 | 0.05817 | 0 | 19.396 | – |
| 23:13:53.1 | −42:36:15 | 0.05775 | 0 | 15.123 | – |
| 23:13:54.6 | −42:47:53 | 0.05768 | 1 | 19.654 | – |
| 23:13:54.7 | −42:41:18 | 0.06083 | 0 | 17.371 | – |
| 23:13:54.9 | −42:43:57 | 0.05672 | 0 | 18.315 | – |
| 23:13:57.2 | −42:41:39 | 0.05463 | 0 | 15.999 | – |
| 23:13:58.0 | −42:37:11 | 0.05833 | 0 | 19.949 | – |
| 23:13:58.6 | −42:43:39 | 0.05651 | 0 | 14.537 | – |
| 23:14:00.3 | −42:52:07 | 0.05602 | 0 | 18.986 | – |
| 23:14:01.3 | −42:44:26 | 0.06196 | 0 | 16.000 | – |
| 23:14:03.4 | −42:29:47 | 0.05696 | 0 | 17.321 | – |
| 23:14:03.5 | −42:43:11 | 0.05778 | 0 | 17.559 | – |
| 23:14:04.3 | −42:38:05 | 0.05330 | 1 | 16.823 | – |
| 23:14:04.3 | −42:38:24 | 0.05737 | 0 | 17.827 | – |
| 23:14:11.3 | −42:36:40 | 0.05365 | 1 | 20.911 | – |
| 23:14:16.5 | −42:43:16 | 0.05499 | 0 | 17.490 | – |
| 23:14:21.0 | −42:45:01 | 0.05713 | 0 | 17.205 | – |
| 23:14:22.1 | −42:35:10 | 0.05266 | 0 | – | – |
| 23:14:23.0 | −42:39:01 | 0.05449 | 0 | 17.238 | – |
| 23:14:25.5 | −42:40:47 | 0.05693 | 0 | 15.714 | – |
| 23:14:25.6 | −42:33:27 | 0.05558 | 1 | 17.465 | – |
| 23:14:26.9 | −42:42:28 | 0.05604 | 0 | 16.157 | – |
| 23:14:33.6 | −42:20:30 | 0.05402 | 0 | 17.025 | Shectman et al. (1996) |
| 23:14:36.8 | −42:42:51 | 0.05890 | 0 | 17.785 | – |
| 23:14:49.9 | −42:44:24 | 0.06118 | 1 | 19.876 | – |
| 23:14:59.5 | −42:47:46 | 0.05666 | 0 | 19.153 | – |
| 23:15:00.9 | −42:59:54 | 0.05667 | 1 | 17.837 | – |
| 23:15:14.7 | −42:07:40 | 0.05430 | 99 | – | Shectman et al. (1996) |
| 23:15:30.9 | −42:29:14 | 0.05486 | 99 | 16.274 | Zabludoff & Mulchaey (1998) |
| 23:15:52.0 | −42:21:24 | 0.05396 | 1 | 16.590 | – |
| 23:16:31.5 | −42:23:33 | 0.05757 | 99 | – | Shectman et al. (1996) |
| 23:17:02.3 | −42:24:41 | 0.05349 | 0 | – | Shectman et al. (1996) |
Notes. Columns 1, 2 show object positions based on GSC2.3 astrometry. The spectroscopic redshift is given in Col. 3. Column 4 refers to the spectral type: 0 for passive spectra without emission lines, 1 for spectra with undoubtful [OII] or [OIII] lines, and 99 where poor data quality or the absence of spectra hampered classification. We assess a global uncertainty of our redshift measurements of Δz ~ 0.00007 (or v ~ 22 km s-1, see Sect. 3.1). We note that 376 out of the 403 individual sources with spectroscopic redshifts are within the field of our VIMOS pre-imaging. Column 5 gives the R-band magnitude in the Vega system for those sources from the VIMOS pre-imaging. Column 6 lists the references of the NED provided redshifts.
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