Open Access

Table D.2.

Same as Table D.1, but for the quiescent selection of galaxies.

log10(M/M)∈ (8.5, 8.8) (8.8, 9.1) (9.1, 9.5) (9.5, 10.0) (10.0, 11.0) (11.0, 12.0)

0.01 < z < 0.33 224 154 163 160 [195] 238 [388] 18 [73]
0.33 < z < 0.86 976 [1346] 729 [867] 761 [954] 1164 [1371] 3281 [3670] 585 [805]
0.86 < z < 1.00 292 [350] 249 325 462 [513] 1534 [1631] 223 [367]
1.00 < z < 1.60 201 [852] 241 [517] 366 [568] 675 [1086] 3878 [5113] 608 [917]
1.60 < z < 2.30 6 33 53 177 [274] 1860 [2591] 242 [335]
2.30 < z < 2.90 3 6 15 53 676 [859] 90 [102]
2.90 < z < 4.10 24 65 116 133 [181] 452 [488] 96 [101]
4.10 < z < 4.70 11 27 76 86 [133] 108 71
4.70 < z < 5.30 6 18 37 73 357 34
5.30 < z < 6.00 0 2 14 20 91 26

Notes. The selection is made using a rest-frame two-color NUV − r versus R − J criterion (Ilbert et al. 2013; Arnouts et al. 2013).

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