Table 2
Global properties of the cluster sample.
| Cluster | R200 |
|
L200 | N200 | N (1 Mpc) | M/L |
( Mpc) |
( ) |
( ) |
(h70M⊙/L⊙) | |||
|
|
||||||
| MS 0015.9+1609 | 2.33 ± 0.13 | 3.27 ± 0.58 | 17.2 ± 1.6 | 135 ± 12 | 69 ± 8 | 190 ± 51 |
| MS 0451.6–0305 | 1.92 ± 0.12 | 1.84 ± 0.35 | 10.8 ± 1.2 | 81 ± 9 | 48 ± 7 | 170 ± 52 |
| RXC J0856.1+3756 | 1.65 ± 0.10 | 1.0 ± 0.175 | 5.1 ± 0.7 | 48 ± 7 | 28 ± 5 | 197 ± 63 |
| RX J0943.0+4659 | 1.77 ± 0.80 | 1.18 ± 0.25 | 13.6 ± 1.4 | 100 ± 11 | 64 ± 8 | 87 ± 28 |
| RXC J1003.0+3254 | 1.69 ± 0.11 | 0.94 ± 0.20 | 4.8 ± 0.9 | 28 ± 5 | 29 ± 5 | 198 ± 81 |
| RX J1120.1+4318 | 1.46 ± 0.14 | 0.75 ± 0.26 | 8.2 ± 1.2 | 52 ± 7 | 46 ± 7 | 91 ± 45 |
| RXC J1206.2–0848 | 2.03 ± 0.10 | 1.93 ± 0.29 | 17.4 ± 1.7 | 111 ± 11 | 54 ± 7 | 111 ± 27 |
| MS 1241.5+1710 | 1.88 ± 0.13 | 1.78 ± 0.38 | 8.0 ± 1.1 | 55 ± 8 | 30 ± 6 | 224 ± 79 |
| RX J1347.5–1145 | 2.40 ± 0.10 | 3.27 ± 0.40 | 13.9 ± 1.4 | 99 ± 10 | 42 ± 7 | 235 ± 53 |
| MS 1621.5+2640 | 1.90 ± 0.11 | 1.57 ± 0.26 | 7.9 ± 1.0 | 63 ± 8 | 37 ± 6 | 199 ± 59 |
| RX J2228.5+2036 | 1.68 ± 0.12 | 1.09 ± 0.24 | 16.0 ± 1.9 | 117 ± 13 | 58 ± 8 | 68 ± 23 |
Notes. The radius R200 and the 2D projected mass are derived from the weak-lensing analysis. The optical luminosity L200 and the galaxy number N200 are measured inside the radius R200 and are corrected for the background contamination. The total luminosity has been corrected for the incompleteness at faint magnitudes. For comparison, we also give the number of cluster members inside a physical radius of 1 Mpc, N (1 Mpc). The global M/L ratio is given in solar units in the r′-band.
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