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Table 3

Spectroscopic redshifts of cluster member galaxies.

ID α (J2000) δ (J2000) z spec dX [″] Features
XMMU J0302.2-0001
1 (BCG) 03:02:12.260 –00:01:33.87 1.1848 ± 0.0007 5.4 [O ii]†, Ca-K, 4000 Å break
2 03:02:11.462 –00:01:32.01 1.1735 ± 0.0007 7.0 Mg ii, Ca-H/K, 4000 Å break
3 03:02:16.181 –00:03:32.28 1.1806 ± 0.0004 134.3 [O ii], Ca-H/K†
4 03:02:11.774 –00:01:32.61 1.1968 ± 0.0007 2.5 Mg ii, [O ii], Ca-H, G band
5 03:02:09.930 –00:01:05.91 1.2042 ± 0.0004 41.0 [O ii]†
6 03:02:15.228 –00:01:49.87 1.1596 ± 0.0004 52.3 [O ii]
XMMU J1532.2-0836
1 (BCG) 15:32:13.294 –08:37:00.75 1.3592 ± 0.0016 5.5 Mg ii, Ca-H/K
2 15:32:13.149 –08:36:57.97 1.3580 ± 0.0007 2.1 Fe ii, Mg ii, Ca-H/K
3 15:32:13.010 –08:36:57.14 1.3568 ± 0.0005 0.4 Fe ii, [O ii], [Ne iii], [Ne v]

Notes. The last column lists the main detected spectral features. Forbidden lines are detected in emission, the rest in absorption. The distance from the X-ray center in arcseconds is given as the dX parameter.

(†)

The feature is faint.

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