Table 3.
Number of galaxies in the different environments (clusters in superclusters (S), clusters not in superclusters (NS), and field) and above the magnitude and mass completeness limits, in three redshift bins.
Environment | 0.1 ≤ z < 0.2 | 0.2 ≤ z < 0.3 | 0.3 ≤ z ≤ 0.5 | All | |||||
---|---|---|---|---|---|---|---|---|---|
r ≤ 20 | M* > 109.5 | r ≤ 20 | M* > 1010.3 | r ≤ 20 | M* > 1010.8 | r ≤ 20 | M* > Mlim | ||
Clusters (S) | 16 | 20 | 32 | 68 | |||||
Ngal virial | 359 (571) | 348 (554) | 106 (146) | 99 (137) | 67 (152) | 57 (132) | 532 (869) | 504 (823) | |
Ngal outer | 454 (735) | 412 (670) | 136 (186) | 104 (142) | 100 (201) | 80 (165) | 690 (1122) | 596 (977) | |
Clusters (NS) | 8 | 17 | 18 | 43 | |||||
Ngal virial | 71 (142) | 65 (133) | 144 (191) | 122 (161) | 51 (67) | 46 (60) | 266 (400) | 233 (354) | |
Ngal outer | 103 (185) | 102 (183) | 193 (270) | 127 (182) | 57 (77) | 44 (56) | 353 (532) | 273 (421) | |
Field | |||||||||
Ngal | 5145 (9793) | 4511 (8577) | 6911 (10808) | 4615 (7181) | 4502 (7405) | 3125 (5180) | 16558 (28006) | 12251 (20938) |
Notes. Galaxies in clusters are further subdivided into virial and outer members. The quantities in parentheses refer to the number of galaxies weighted for spectroscopic completeness.
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