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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 1015h−1M); (12): cluster total luminosity (in 1012h−2L); (13): mass-to-light ratio (in hM/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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