Table 1.
Seven clusters of this study.
| Cluster | z | RA | Dec | R200 | M200 | Cluster | SF cluster | Members |
|---|---|---|---|---|---|---|---|---|
| name | (Mpc) | (1014 M⊙) | membersa | membersa | with O/Ha | |||
| RXJ1720 | 0.1599 | 17:20:10.14 | +26:37:30.90 | 2.02 | 9.40 | 358/219 | 63/22 | 45/15 |
| A1914 | 0.1671 | 14:25:59.78 | +37:49:29.10 | 1.90 | 7.69 | 388/276 | 101/50 | 65/31 |
| A1689 | 0.1851 | 13:11:29.45 | −01:20:28.30 | 2.13 | 11.01 | 438/291 | 116/46 | 66/32 |
| A963 | 0.2043 | 10:17:01.20 | +39:01:44.40 | 1.81 | 6.75 | 414/332 | 107/75 | 69/45 |
| A2390 | 0.2291 | 21:53:36.72 | +17:41:31.20 | 2.21 | 12.36 | 371/287 | 86/70 | 61/48 |
| A1763 | 0.2323 | 13:35:16.32 | +40:59:45.60 | 1.85 | 7.18 | 292/230 | 76/63 | 53/43 |
| A1835 | 0.2520 | 14:01:02.40 | +02:52:55.20 | 2.27 | 13.34 | 465/330 | 112/84 | 62/45 |
Notes.
The table lists: mean redshift of cluster members, coordinates, radii R200 and cluster masses M200 (as reported in Haines et al. 2013); number of cluster members, star-forming (SF) objects and galaxies with O/H measured in our sample. The “200” subscript refers to the radius where the average density is 200 times the critical density of the Universe at the cluster redshift.
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