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Table 4

Same as Table 3 but for C3 XMM-LSS systems.

Name XLSSC  PH RA Dec N ZBWT ERRZ SIG ERR Flux [0.5;2] keV L Bol N NP Lit Id Lit z
deg deg km s-1 km s-1 10-14 erg/cm2/s 1043erg/s
in 0.5 Mpc in 0.5 Mpc in 0.5 Mpc

XLSSU J021651.3-042328* 1 34.214 −4.392 1 0.273 0.6  ±  0.3 0.3  ±  0.2 58  ±  32
XLSSU J021754.6-052655(l) 066 1 34.478 −5.447 6 0.250 0.3  ±  0.3 0.1  ±  0.1 68  ±  59 SXDF85XGG/621 0.25
XLSSU J021842.8-053254 067 1 34.678 −5.548 5 0.380 0.001 847 279 1.0  ±  0.4 1.0  ±  0.4 84  ±  34 SXDF01XGG/876 0.378
XLSSU J021940.3-045103* 1 34.919 −4.852 1 0.454 0.8  ±  0.2 1.2  ±  0.3 193  ±  44
XLSS J022258.4-04070 024 1 35.744 −4.121 5 0.293 0.001 452 98 1.3  ±  0.2 0.7  ±  0.1 254  ±  41
XLSS J022341.8-043051 026 1 35.925 −4.514 3 0.436 1.6  ±  0.2 2.2  ±  0.3 255  ±  34
XLSSU J022509.2-043239 037 1 36.286 −4.542 3 0.767 0.1  ±  0.1 0.3  ±  0.7 11  ±  28
XLSSU J022510.5-040147 043** 1 36.294 −4.029 3 0.170 2.6  ±  0.9 0.4  ±  0.1 142  ±  49
XLSS J022522.8-042649 042 1 36.345 −4.447 6 0.462 0.003 1009 257 0.6  ±  0.2 0.9  ±  0.3 111  ±  33
XLSS J022542.2-042434 068 1 36.424 −4.410 4 0.585 0.2  ±  0.2 0.5  ±  0.6 23  ±  28
XLSS J022610.0-043120 069 1 36.542 −4.523 8 0.824 0.001 398 114 −0.4  ±  0.2
XLSSU J022627.3-050001 017 1 36.615 −5.003 5 0.383 0.001 352 132 1.5  ±  0.4 1.6  ±  0.4 134  ±  35
XLSSU J022632.5-040314 014 1 36.635 −4.054 6 0.345 0.001 304 84 1.4  ±  0.5 1.1  ±  0.4 74  ±  29
XLSSU J022632.4-050003 020 1 36.638 −5.007 3 0.494 2.0  ±  0.4 3.8  ±  0.8 159  ±  32
XLSSU J022726.8-045412 070 1 36.860 −4.904 5 0.301 0.001 180 47 0.2  ±  0.2 0.1  ±  0.1 32  ±  39
XLSS J022754.1-035100* 1 36.974 −3.851 2 0.140 0.7  ±  0.5 0.1  ±  0.1 107  ±  72
XLSSU J022828.9-045939 016* 1 37.121 −4.994 2 0.335 0.4  ±  0.5 0.3  ±  0.4 33  ±  44

C555 1 36.375 −4.429 7 0.921 0.001 759 248 0.3  ±  0.1 2.9  ±  1.1 47  ±  18

Notes. The ** symbols indicate that we merged by hand two groups separated by the gapper technique in the final analysis. The last line (C555 class) is the new cluster (see text). The * symbols indicate that the cluster validation was made with one or two spectroscopic redshifts. The (l) attached to the cluster id means that we have a lack of precision in the measured galaxy redshifts, which prevents us from computing the uncertainty of the mean cluster redshift and the velocity dispersions.

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