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Table 1

Comparison clusters and A 520 with their main parameters.

Cluster z N m σ v R 200 M 200 N pass N sf N rq N AGN
(km s-1) (Mpc) [1014M] (%) (%) (%) (%)

A665 0.1818 310(360) 1268 2.87 21.5 205(66) 100(32) 14(4) 5(5)
A1689 0.1832 519(934) 1779 4.02 59.2 308(59) 185(35) 24(4) 26(12)
A383 0.1883 164(260) 898 2.02 7.6 88(53) 63(38) 23(14) 13(17)
A291 0.196 131(131) 682 1.53 3.3 79(60) 46(35) 0(0) 6(12)
A963 0.205 414(492) 1199 2.68 17.9 206(49) 199(48) 21(5) 9(4)
Z1693 a 0.2248 212(265) 683 1.51 3.3 129(60) 74(34) 16(7) 9(11)
A1763 0.2279 305(447) 1399 3.09 28.1 156(51) 122(40) 38(12) 27(18)
A2390 0.2329 356(552) 1336 2.94 24.4 193(54) 135(37) 5(1) 28(17)
Z2089 b 0.2347 141(141) 761 1.68 4.5 80(56) 50(35) 14(9) 11(18)
R2129 c 0.235 236(307) 907 2.00 7.6 148(62) 74(31) 16(6) 14(16)
A 520 0.2007 190(315) 1036 2.32 11.6 137(72) 50(26) 12(6) 3(5)

Notes. Nm is the number of cluster members from the ACReS survey (combined data set) or in the case of A 520 from the MMT data set (full data set). Npass, Nsf and Nrq are the number (fraction) of passive, star forming and recently quenched galaxies, respectively. NAGN is the number (fraction) of emission-line galaxies who’s spectra are dominated by AGN emission. All the numbers and fractions are calculated among all the members of the given cluster.

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