Table 1.
Data on rich galaxy clusters in the Coma and Leo superclusters based on SDSS DR10.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| No. | Abell ID | ID | Ngal | RA | Dec | z | σv | Rg | Rmax | MNFW | Ltot | M/L | D8 |
| 1 | A1656 | 52 | 680 | 194.7 | 27.9 | 0.024 | 840 | 0.68 | 2.7 | 0.91 | 2.55 | 357 | 11.7 |
| 2 | A1367 | 90 | 245 | 176.2 | 20.0 | 0.023 | 685 | 0.51 | 2.0 | 0.46 | 1.15 | 400 | 8.5 |
| 3 | A1185 | 607 | 211 | 167.6 | 28.4 | 0.034 | 610 | 0.61 | 2.2 | 0.47 | 1.15 | 409 | 6.4 |
Notes. Columns are as follows: (1): Order number of the cluster; (2): Abell ID number of the cluster; (3): ID of the cluster from Tempel et al. (2014a); (4): Number of galaxies in the cluster, Ngal; (5)–(6): cluster centre right ascension and declination (in degrees); (7): redshift of the cluster; (8): line-of-sight velocity dispersion of cluster member galaxies, in km s−1; (9): cluster gravitational radius Rg (in h−1 Mpc); (10): maximum radius of a cluster in the plane of the sky (in h−1 Mpc); (11): mass of the cluster assuming an NFW density profile, MNFW (in 1015 h−1 M⊙); (12): cluster total luminosity (in 1012 h−2 L⊙); (13): mass-to-light ratio (in h M⊙/L⊙); (14): luminosity-density field value at the location of the cluster, D8, in units of the mean density as described in the text.
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