Table 2
Properties of the newly discovered or with newly published individual member redshifts, XDCP clusters selected for our study.
| Cluster ID | RA | Dec | z | Follow-up |
|
|
|
Program ID | ||||
| J2000 | J2000 | color | (km s-1) | (1044 erg s-1) | ||||||||
|
|
||||||||||||
| XDCP J1450.1+0904 – cl01* | 14:50:09.2 | +09:04:39.1 | 0.642 | R − z | 13 | 414 | ± | 136 | 1.05 | ± | 0.20 | 085.A-0647(B) |
| XDCP J1119.1+1300 – cl02 | 11:19:07.7 | +13:00:23.8 | 0.676 | z − H | 13 | 499 | ± | 87 | 0.35 | ± | 0.09 | 079.A-0634(D) |
| XDCP J1044.7−0119 – cl03 | 10:44:43.7 | −01:19:54.3 | 0.755 | R − z | 17 | 795 | ± | 188 | 1.70 | ± | 0.60 | 085.A-0647(B) |
| XDCP J0002.2−3556 – cl04 | 00:02:16.1 | −35:56:33.8 | 0.770 | z − H | 13 | 1089 | ± | 144 | 2.00 | ± | 0.25 | 081.A-0332(B) |
| XDCP J1243.2+1313 – cl05 | 12:43:12.0 | +13:13:09.6 | 0.791 | R − z | 25 | 840 | ± | 139 | 1.70 | ± | 0.50 | 084.A-0844(B) |
| XDCP J0954.2+1738 – cl06 | 09:54:17.1 | +17:38:05.9 | 0.828 | R − z, z − H | 10 | 992 | ± | 175 | 6.70 | ± | 0.75 | 084.A-0844(B) |
| XDCP J0010.7−1127 – cl07 | 00:10:42.4 | −11:27:46.0 | 0.828 | R − z | 15 | 416 | ± | 74 | 10.30 | ± | 1.60 | 080.A-0659(A) |
| XDCP J0152.6−1338 – cl08* | 01:52:41.3 | −13:38:54.3 | 0.829 | z − H | 12 | 483 | ± | 98 | 2.50 | ± | 0.50 | 084.A-0844(B) |
| XDCP J2356.2−3441 – cl09 | 23:56:16.5 | −34:41:41.8 | 0.939 | z − H | 20 | 624 | ± | 146 | 6.50 | ± | 1.50 | 081.A-0332(B) |
| XDCP J2215.9−1751 – cl10† | 22:15:56.9 | −17:51:40.9 | 1.224 | z − H | 10 | 493 | ± | 114 | 0.55 | ± | 0.07 | 080.A-0659(A) |
Notes. The 5th column reports the imaging color(s) used for the photometric identification. The last column provides the identification codes of the used spectroscopic FORS2 programs.
Clusters cl01 and cl08 are published in the XMM Cluster Survey – Data Release 1 (XCS-DR1). Specifically, for cl01 a consistent photometric redshift of z = 0.60 is provided in the XCS-DR1 web page table, accessible from http://xcs-home.org/datareleases. The X-ray and spectroscopic properties of cl08 are, instead, discussed in Mehrtens et al. (2012). In both cases, however, the detailed lists of member redshifts were not provided before this work.
The system XDCP J2215.9−1751 was previously published in Fassbender et al. (2011a) and de Hoon et al. (2013), but here we provide the value of σv and perform its kinematic analysis.
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