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Table 2

Cluster sample details.

Bin N200 nclus z N200 σlnM | N200 M200 c200 b σs pc cgal Agal
Mpc] []
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

0.20 < z < 0.35
N1z1 2.00–7.63 534 0.30 5.2 4.0 0.57
N2z1 7.63–10.47 345 0.28 9.0 7.5 0.47
N3z1 10.47–13.65 268 0.27 11.9 10.4 0.46
N4z1 13.65–18.14 216 0.27 15.8 14.3 0.46
N5z1 18.14–26.31 197 0.25 21.8 21.2 0.47
N6z1 26.31–220.00 114 0.24 38.0 36.6 0.57
0.35 < z < 0.55
N1z2 2.00–7.63 1648 0.47 5.0 4.0 0.59
N2z2 7.63–10.47 607 0.46 8.9 7.7 0.47
N3z2 10.47–13.65 326 0.46 11.9 10.5 0.46
N4z2 13.65–18.14 216 0.47 15.7 14.2 0.46
N5z2 18.14–26.31 126 0.46 21.2 19.5 0.47
N6z2 26.31–220.00 59 0.46 36.9 34.0 0.56
0.55 <z< 0.80
N1z3 2.00–7.63 1170 0.64 5.1 3.3 0.58
N2z3 7.63–10.47 670 0.66 9.0 6.6 0.46
N3z3 10.47–13.65 512 0.67 11.9 9.4 0.46
N4z3 13.65–18.14 340 0.67 15.5 13.0 0.46
N5z3 18.14–26.31 190 0.67 21.3 20.1 0.47
N6z3 26.31–220.00 73 0.68 36.0 33.1 0.55

Notes. (1) richness range of the bin; (2) number of clusters; (3) median redshift; (4) mean richness; (5) mean richness corrected for Eddington bias; (6) prior-mean of the scatter in the mass-richness relation; (7) halo mass; (8) concentration; (9) halo bias; (10) miscentring width; (11) centring fraction; (12) concentration of satellite distribution; (13) amplitude of cluster-satellite correlation.

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