Table 1.
Stacked clusters.
| Method | Nmin | r200 | log M200 | log rE | log rS0 | log rS | Number (all) | Number (Rmin ↔ Rmax) | ||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (kpc) | (M⊙) | (kpc) | (kpc) | (kpc) | Total | E | S0 | S | Total | E | S0 | S | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
| sigv | 30 | 1749 | 14.79 | 2.690 ± 0.097 | 2.813 ± 0.107 | 3.314 ± 0.105 | 4816 | 1701 | 1871 | 1244 | 4682 | 1607 | 1845 | 1230 |
| sigv | 81 | 1846 | 14.86 | 2.708 ± 0.128 | 2.813 ± 0.087 | 3.322 ± 0.122 | 3361 | 1164 | 1334 | 863 | 3289 | 1109 | 1321 | 859 |
| Num | 30 | 1629 | 14.69 | 2.690 ± 0.106 | 2.799 ± 0.103 | 3.270 ± 0.103 | 4730 | 1676 | 1838 | 1216 | 4593 | 1583 | 1807 | 1203 |
| tempX | 30 | 1710 | 14.76 | 2.602 ± 0.152 | 2.699 ± 0.078 | 3.369 ± 0.126 | 3607 | 1264 | 1441 | 902 | 3523 | 1198 | 1426 | 899 |
Notes. Columns are as follows. (1): stacking method; (2): minimum number of galaxies per cluster; (3): r200 obtained from Clean; (4): log M200 corresponding to r200; (5–7): scale radii of the spatial distributions of elliptical (5), lenticular (6), and spiral (7) galaxies, determined from fits of the photometric data; (8–11): total number of galaxies in sample; (12–15): number of galaxies restricted to the projected radii analyzed by MAMPOSSt.
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