Table 3
Results on galaxy clusters.
| Cluster | z |
|
n bg |
|
σNFW/σ2D |
|
|
|
| (arcmin-2) | (kpc  ) |
|
|
|
||||
|
|
||||||||
| XDCS0329 | 0.4122 | 0.90 | 10.20 | – | 1.2/2.8 | – | – | 2.9 ± 0.6 |
| MACSJ0454 | 0.5377 | 0.99 | 9.96 | – | 1.9/5.1 | – | – | 13.9 ± 3.0 |
| ABELL0851 | 0.4069 | 0.92 | 8.30 | 1542 ± 160 | 3.9/7.6 | 6.6 ± 2.0 | 4.4 ± 1.4 | 5.5 ± 1.2 |
| LCDCS0829 | 0.4510 | 0.93 | 8.79 | 1638 ± 218 | 3.8/5.5 | 8.5 ± 3.2 | 5.7 ± 2.1 | 16.9 ± 3.6 |
| MS1621 | 0.4260 | 0.93 | 14.13 | 1718 ± 140 | 6.4/8.3 | 9.2 ± 2.2 | 6.2 ± 1.5 | 4.5 ± 0.5M12 |
| OC02 | 0.4530 | 0.96 | 13.15 | 1202 ± 187 | 3.1/4.7 | 3.4 ± 1.5 | 2.3 ± 1.0 | – |
| NEP200 | 0.6909 | 1.02 | 5.80 | 1929 ± 306 | 3.3/5.1 | 18.9 ± 8.2 | 12.7 ± 5.5 | – |
| RXJ2328 | 0.4970 | 0.95 | 11.46 | 1393 ± 159 | 3.2/5.5 | 5.5 ± 1.9 | 3.7 ± 1.2 | 2.2 ± 0.5 |
| CLJ0152 | 0.8310 | 1.19 | 14.94 | 1670 ± 194 | 3.8/8.3 | 14.0 ± 4.6 | 9.4 ± 3.1 | 8.8 ± 1.9 |
| MACSJ0717 | 0.5458 | 0.98 | 13.16 | 2236 ± 206 | 5.2/10.9 | 23.6 ± 6.4 | 15.9 ± 4.3 | 17.8 ± 1.7M12 |
| BMW1226 | 0.8900 | 1.43 | 10.12 | – | 0.2/ – | – | – | 12.1 ± 0.4 |
| MACSJ1423 | 0.5450 | 0.93 | 8.98 | 1594 ± 214 | 3.4/5.0 | 8.8 ± 3.3 | 5.9 ± 2.2 | 5.7 ± 1.2 |
| MACSJ1621 | 0.4650 | 0.94 | 16.39 | 1379 ± 185 | 4.2/6.8 | 5.2 ± 1.9 | 3.5 ± 1.3 | 4.3 ± 0.4M12 |
| RXJ1716 | 0.8130 | 1.17 | 7.49 | 1685 ± 194 | 3.9/7.3 | 14.1 ± 4.7 | 9.5 ± 3.2 | 2.8 ± 0.5M12 |
| MS2053* | 0.5830 | 0.98 | 14.44 | 1620 ± 195 | 4.6/8.7 | 9.5 ± 3.3 | 6.4 ± 2.2 | 4.9 ± 1.1 |
| CXOSEXSI2056* | 0.6002 | 0.98 | 14.44 | – | 0.7/4.4 | – | – | 3.6 ± 0.8 |
Notes. The first eight clusters are observed with CFHT/Megacam and the last eight with Subaru/Suprime-cam. The different columns correspond to #1: cluster ID; #2: cluster redshift; #3: mean redshift of background galaxies; #4: mean galaxy density of the background galaxies; #5: r200 from the best NFW fit; #6: significance of the NFW fit/significance of the WL peak in the 2D mass map; #7: from the best NFW fit centered on the WL peak; #8: computed in r500 from , assuming the same NFW profile; and #9: total masses in r500 derived from XMM X-ray data from Guennou et al. (2014) or Chandra X-ray data from the Maughan et al. (2012) sample denoted by the symbol M12 and computed in Laganá et al. (2013).
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