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Table 2

Data on groups in the A2142 supercluster with at least ten member galaxies.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

No. ID Ngal R.A. Dec. Dist. σv rmax Ltot Mdyn M/L D8
[deg] [deg] [h-1 Mpc] [km s-1] [h-1 Mpc] [1010h-2L] [1012h-1M] [hM/L]

1 10570 27 238.53 27.47 268.57 247.76 1.26 51.3 59.5 116.2 13.65
2 3070 212 239.52 27.32 264.64 769.02 2.39 382.0 906.5 237.3 20.70
3 4952 54 239.78 26.56 260.11 447.24 1.30 111.0 214.4 193.1 17.13
4 32074 11 240.11 26.71 262.42 337.05 0.61 15.7 59.5 378.2 19.89
5 35107 10 240.13 27.01 258.69 221.02 0.77 13.9 30.3 218.4 14.20
6 14960 27 240.20 25.87 263.58 382.58 1.30 46.6 147.5 316.6 15.32
7 17779 20 240.38 26.16 261.06 371.74 1.15 35.1 104.1 296.9 16.39
8 6885 32 240.75 25.40 258.85 428.12 1.22 70.5 164.1 232.8 11.38
9 21183 21 240.83 26.95 265.02 280.10 1.29 36.5 61.2 167.6 15.20
10 20324 11 240.95 24.95 259.72 335.77 0.73 17.4 77.5 446.2 10.42
11 10818 28 241.23 24.52 259.56 328.02 1.29 51.3 105.1 205.1 9.31
12 14283 19 241.90 23.21 260.28 323.03 0.86 34.4 65.1 189.0 7.27
13 10224 32 242.91 21.02 254.55 633.40 0.86 60.4 232.5 385.0 6.01
14 26895 12 243.08 20.77 254.80 257.42 0.92 16.5 49.1 297.9 5.91

Notes. Columns are as follows: (1): Order number of the group; (2): ID of the group from Tempel et al. (2014b) (Gr 3070 correspond to the Abell cluster A2142); (3): the number of galaxies in the group, Ngal; (4)–(5): group center right ascension and declination; (6): group center comoving distance; (7): rms velocity of galaxies in the group; (8): group maximum radius; (9): group total luminosity; (10): dynamical mass of the group assuming the NFW density profile, Mdyn; (11): group mass-to-light ratio M/L; (12): the value of the luminosity-density field at the location of the group calculated with the 8h-1Mpc smoothing length, D8, in units of the mean density as described in the text.

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