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Table A.1

Spectroscopic details of the galaxies of the cluster cl01.

R 500 RA Dec z z err QF Distance from X-ray centroid Clipped
(kpc) (J2000) (J2000) (′′) (kpc) (r/R500) out

XDCP J1450.1+0904 – cl01

644 14:50:09.2 +09:04:39.1 0.6417

14:50:09.3 +09:04:39.2 0.6419 0.0002 3 1 6 0.009
14:50:09.2 +09:04:45.1 0.6425 0.0002 3 6 42 0.065
14:50:10.4 +09:04:23.5 0.6418 0.0002 2 23 160 0.248
14:50:09.5 +09:04:15.9 0.6430 0.0002 3 24 163 0.253
14:50:07.4 +09:04:28.7 0.6429 0.0002 3 28 192 0.298
14:50:09.3 +09:04:06.5 0.6377 0.0002 3 33 225 0.349
14:50:10.4 +09:03:53.3 0.6462 0.0003 2 49 339 0.526
14:50:10.6 +09:05:32.4 0.6379 0.0002 3 57 394 0.612
14:50:13.8 +09:03:21.9 0.6407 0.0002 3 103 707 1.098
14:50:16.0 +09:02:57.5 0.6420 0.0002 2 143 984 1.528
14:50:04.9 +09:06:55.0 0.6405 0.0002 3 150 1032 1.602

Notes. The “QF” column reports the quality flag associated to each spectroscopic redshift with QF = 2, 3, and 4 corresponding to a confidence level for the estimated z value of >75%, >90%, and 100%, respectively, whereas QF = 1 is for tentative estimates. A check mark symbol in the last column indicates that the object has been rejected as cluster member by the σ-clipping procedure described in the text. All objects with QF = 1 are excluded from the analysis.

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