Table 3
Properties of the BCGs.
BCG | RA | Dec | z | (g − r) | M r | Mass |
Clus-no. | (2000) | (2000) | 1011 M⊙ | |||
|
||||||
XLSSC 081 | 33.0515 | –6.21080 | 0.4266 ± 0.0006 | 1.53 | –21.61 | 7.7 |
XLSSC 082 | 32.7140 | –6.17883 | 0.4240 ± 0.0005 | 1.42 | –21.76 | 6.7 |
XLSSC 083 | 32.7350 | –6.19845 | 0.4303 ± 0.0007 | 1.59 | –21.80 | 10.6 |
XLSSC 084 | 32.7621 | –6.21303 | 0.4324 ± 0.0004 | 1.51 | –21.04 | 4.2 |
XLSSC 085 | 32.8697 | –6.19631 | 0.4289 ± 0.0008 | 1.56 | –22.27 | 15.1 |
XLSSC 086 | 32.8081 | –6.16231 | 0.4257 ± 0.0006 | 1.39 | –21.51 | 4.9 |
Notes. We list the BCG group ID, their coordinates, the redshift for each galaxy, the observed colour (corrected for extinction), their absolute magnitude in r band, and mass derived from the analysis of the optical data. The mass was obtained using the M − L relation from Bell et al. (2003); an uncertainty of 10% should be assumed on the mass estimate.
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