Table 4
Comparison of masses centered on the WL peak and on the BCG for 11 clusters.
| Cluster |
|
θ | WL−BCG | |
|
|
(kpc  ) |
(arcmin) |
|
|
|
|
|
||||
| ABELL0851 | 384 | 1.18 | 6.6 ± 2.0 | 2.5 ± 1.6 |
| LCDCS0829 | 178 | 0.51 | 8.5 ± 3.2 | 6.5 ± 2.9 |
| MS1621 | 338 | 1.01 | 9.2 ± 2.2 | 5.6 ± 1.8 |
| OC02 | 74 | 0.21 | 3.4 ± 1.5 | 2.8 ± 1.4 |
| NEP200 | 209 | 0.49 | 18.9 ± 8.2 | 8.4 ± 5.2 |
| RXJ2328 | 343 | 0.94 | 5.5 ± 1.9 | 3.2 ± 1.8 |
| CLJ0152 | 339 | 0.74 | 14.0 ± 4.6 | 9.5 ± 4.3 |
| MACSJ1423 | 146 | 0.38 | 8.8 ± 3.3 | 7.2 ± 3.3 |
| MACSJ1621 | 422 | 1.20 | 5.2 ± 1.9 | 1.7 ± 1.1 |
| RXJ1716 | 190 | 0.42 | 14.1 ± 4.7 | 12.9 ± 4.5 |
| MS2053 | 87 | 0.29 | 9.5 ± 3.3 | 8.6 ± 2.9 |
Notes. The first six clusters are observed with CFHT/Megacam and the last five with Subaru/Suprime-cam. The different columns correspond to #1: cluster ID; #2: comoving distance between the WL peak and the BCG in kpc; #3: θ| WL−BCG | angular distance between the WL peak and the BCG in arcmin; #4: from the best NFW fit centered on the WL peak; and #5: from the best NFW fit centered on the BCG.
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