Table 1
Cluster properties.
| XLSSC ID | z | M500,WL | M1 Mpc,WL | LK,500 | LK,1 Mpc | M⋆,500 | M⋆,1 Mpc | N500 | |
| (1014 M⊙) | (1014 M⊙) | (1012LK, ⊙) | (1012LK, ⊙) | (1012 M⊙) | (1012 M⊙) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
|
|
|||||||||
| 027 | 0.295 |
|
|
5.1 ± 1.0 | 5.1 ± 1.4 | 3.7 ± 0.8 | 3.7 ± 1.0 | 49 ± 15 | |
| 054 | 0.054 |
|
|
2.2 ± 0.5 | 2.6 ± 1.0 | 1.6 ± 0.4 | 1.9 ± 0.7 | 39 ± 9 | |
| 055 | 0.232 |
|
|
8.3 ± 1.9 | 7.6 ± 1.6 | 6.1 ± 1.4 | 5.5 ± 1.2 | 114 ± 26 | |
| 056 | 0.348 |
|
|
11.1 ± 1.6 | 11.6 ± 1.9 | 8.1 ± 1.2 | 8.5 ± 1.4 | 84 ± 15 | |
| 060 | 0.139 |
|
|
7.3 ± 1.1 | 9.6 ± 1.6 | 5.3 ± 0.8 | 7.0 ± 1.2 | 103 ± 10 | |
| 061 | 0.259 |
|
|
2.7 ± 1.3 | 2.8 ± 1.1 | 2.0 ± 0.8 | 1.9 ± 1.0 | 71 ± 18 | |
| 083 | 0.430 |
|
|
8.5 ± 1.5 | 9.5 ± 1.9 | 6.2 ± 1.1 | 7.0 ± 1.4 | 87 ± 12 | |
| 084 | 0.430 |
|
|
7.5 ± 1.1 | 9.8 ± 1.4 | 5.5 ± 0.8 | 7.1 ± 1.0 | 89 ± 13 | |
| 087 | 0.141 |
|
|
1.0 ± 0.4 | 1.5 ± 1.1 | 0.7 ± 0.3 | 1.1 ± 0.8 | 18 ± 8 | |
| 088 | 0.295 |
|
|
6.9 ± 0.8 | 8.7 ± 1.4 | 5.0 ± 0.6 | 6.3 ± 1.0 | 60 ± 10 | |
| 091 | 0.186 |
|
|
18.0 ± 2.2 | 17.2 ± 1.8 | 13.2 ± 1.6 | 12.5 ± 1.3 | 233 ± 27 | |
| 098 | 0.297 |
|
|
4.0 ± 0.9 | 4.4 ± 1.3 | 2.9 ± 0.7 | 3.2 ± 1.0 | 44 ± 13 | |
| 103 | 0.233 |
|
|
2.5 ± 1.5 | 2.6 ± 1.2 | 1.8 ± 1.1 | 1.9 ± 0.9 | 35 ± 25 | |
| 104 | 0.294 |
|
|
4.3 ± 0.8 | 4.6 ± 1.2 | 3.2 ± 0.6 | 3.4 ± 0.9 | 50 ± 13 | |
| 105 | 0.429 |
|
|
8.8 ± 2.4 | 8.3 ± 1.5 | 6.4 ± 1.7 | 6.0 ± 1.1 | 101 ± 30 | |
| 106 | 0.300 |
|
|
10.9 ± 1.7 | 11.3 ± 1.6 | 8.0 ± 1.2 | 8.2 ± 1.2 | 129 ± 22 | |
| 109 | 0.491 |
|
|
4.4 ± 1.8 | 4.4 ± 1.8 | 3.2 ± 1.3 | 3.2 ± 1.3 | 28 ± 16 | |
| 110 | 0.445 |
|
|
9.3 ± 2.2 | 9.6 ± 1.8 | 7.0 ± 1.3 | 6.8 ± 1.6 | 65 ± 13 | |
| 111 | 0.299 |
|
|
13.2 ± 1.8 | 15.0 ± 2.3 | 11.0 ± 1.7 | 9.7 ± 1.3 | 139 ± 28 | |
| 112 | 0.139 |
|
|
2.3 ± 0.7 | 1.9 ± 1.3 | 1.6 ± 0.5 | 1.4 ± 0.9 | 18 ± 10 | |
Notes. Column 1 shows the cluster identification number; Col. 2 shows the cluster redshift (from Paper II); the weak-lensing masses measured within r500,WL (from Paper IV) and 1 Mpc are shown in Cols. 3 and 4, respectively; Cols. 5 and 6 show the K-band luminosities measured within r500,WL and 1 Mpc from the X-ray centroid of the cluster, respectively; Cols. 7 and 8 are the stellar masses obtained by multiplying the K-band luminosities within r500,WL and 1 Mpc by a fixed mass-to-light ratio of 0.73; Col. 9 is the number of galaxies contributing to the K-band luminosity within r500,WL. The position (right ascension and declination) of these objects can be found in Table 1 of Paper II.
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