Table 1
Spectroscopic dataset.
| Id | α J2000 | δ J2000 | z SDSS | z VIMOS | Member | Subst | Prob |
|
|
|||||||
| 2 |
|
|
0.6056 | – | – | – | – |
| 164 |
|
|
– | 0.1768 | M | – | – |
| 328 |
|
|
0.1748 | – | M | – | – |
| 3272 |
|
|
0.3732 | 0.3719 | – | – | – |
| 3664 |
|
|
– | 0.1734 | M | – | 0.98 |
| 3667 |
|
|
0.1701 | – | M | – | 0.07 |
| 6437 |
|
|
0.1785 | – | M | S | – |
Notes. The average uncertainties in the VIMOS and SDSS redshifts are 3.7 × 10-4 and 1.0 × 10-4, respectively. An “M” in the “Member” column identifies cluster members (identified as described in Sect. 3), and an “S” in the “Subst” column identifies galaxies belonging to DSb-type substructures (see Sect. 4 and Appendix A). The “Prob” column lists probabilities of belonging to the KMM-main subcluster (see Sect. 4). Only a portion of the Table is shown here, the full Table is available in at the CDS.
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