Table 3
Same as Table 2 but for C2 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 J021658.9-044904 | 065 | 1 | 34.245 | −4.821 | 3 | 0.435 | 1.1 ± 0.4 | 1.6 ± 0.6 | 50 ± 18 | 285/287 | ||||
| XLSSU J021832.0-050105 | 064 | 1 | 34.633 | −5.016 | 3 | 0.875 | 1.6 ± 0.1 | 13.5 ± 0.8 | 937 ± 56 | SXDF46XGG/829 | 0.875 | |||
| XLSSU J021837.0-054028 | 063* | 1 | 34.654 | −5.675 | 2 | 0.275 | 4.1 ± 0.5 | 2.0 ± 0.2 | 255 ± 32 | |||||
| XLSS J022303.3-043621 | 046 | 1 | 35.764 | −4.606 | 8 | 1.213 | 0.001 | 595 | 121 | 0.7 ± 0.1 | 14.0 ± 3.2 | 82 ± 19 | ||
| XLSS J022307.2-041259 | 030 | 0 | 35.780 | −4.216 | 5 | 0.631 | 0.001 | 520 | 158 | 0.6 ± 0.1 | 2.1 ± 0.4 | 129 ± 27 | ||
| XLSS J022405.9-035512 | 007 | 1 | 36.024 | −3.920 | 5 | 0.559 | 0.001 | 369 | 179 | 1.2 ± 0.3 | 3.2 ± 0.7 | 113 ± 25 | ||
| XLSSU J022644.2-034107 | 009 | 1 | 36.686 | −3.684 | 8 | 0.328 | 0.001 | 261 | 53 | 1.7 ± 0.4 | 1.2 ± 0.3 | 87 ± 21 | ||
| XLSS J022725.1-041127 | 038 | 1 | 36.854 | −4.191 | 4 | 0.584 | 0.1 ± 0.1 | 0.4 ± 0.3 | 31 ± 28 | |||||
| XLSS J022756.3-043119* | − | 1 | 36.985 | −4.522 | 2 | 1.050? | 0.2 ± 0.1 | 2.9 ± 1.5 | 49 ± 26 | |||||
Notes. XLSS J022756.3-043119 would require more spectroscopy for confirmation. XLSSC 009, 064, and 065 were originally classified as C2, but would be classified as C1 using more recent pipeline version. 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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