Table 5
Results on environment.
| Cluster | z | Structure | σ 2D | Detection | X-ray | Galaxies | Cluster status |
| percentage | |||||||
|
|
|||||||
| XDCS0329 | 0.4122 | 1 | 2.8 | 44% | Y | Y | – |
| 2 | 5.6 | 96% | N | N | |||
| 3 | 3.9 | 74% | N | ~ | |||
| MACSJ0454 | 0.5377 | 1 | 5.1 | 91% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 4.2 | 76% | Y | Y | |||
| 3 | 3.7 | 67% | N | ~ | |||
| 4 | 4.4 | 88% | N | N | |||
| 5 | 3.8 | 70% | N | ~ | |||
| 6 | 4.2 | 82% | N | ~ | |||
| 7 | 4.0 | 78% | N | N | |||
| 8 | 5.5 | 95% | N | N | |||
| ABELL851 | 0.4069 | 1 | 7.6 | 100% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 5.0 | 89% | ~ | Y | |||
| 3 | 4.3 | 81% | ~ | Y | |||
| 4 | 4.4 | 86% | N | N | |||
| LCDCS0829 | 0.4510 | 1 | 5.5 | 98% | Y | Y | past merger (2) |
| 2 | 4.5 | 86% | – | Y | |||
| 3 | 4.7 | 92% | – | Y | |||
| MS1621 | 0.4260 | 1 | 8.3 | 100% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 4.3 | 77% | ~ | Y | |||
| 3 | 3.5 | 67% | N | N | |||
| 4 | 3.1 | 53% | N | N | |||
| OC02 | 0.4530 | 1 | 4.7 | 88% | Y | Y | recent or present merger (3) |
| 2 | 5.8 | 98% | Y | ~ | foreground cluster (A2246) | ||
| 3 | 4.2 | 78% | N | ~ | |||
| NEP200 | 0.6909 | 1 | 5.1 | 93% | Y | Y | recent or present merger (3) |
| 2 | 4.6 | 84% | N | N | |||
| RXJ2328 | 0.4970 | 1 | 5.5 | 93% | Y | Y | recent or present merger (3) |
| 2 | 3.9 | 73% | N | N | |||
| CLJ0152 | 0.8310 | 1 | 8.3 | 100% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 6.4 | 98% | Y | N | |||
| 3 | 4.8 | 85% | Y | N | |||
| 4 | 6.6 | 98% | Y | Y | |||
| 5 | 4.7 | 89% | ~ | N | |||
| MACSJ0717 | 0.5458 | 1 | 10.9 | 100% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 8.2 | 100% | ~ | Y | |||
| 3 | 5.7 | 98% | N | Y | |||
| BMW1226 | 0.8900 | 0 | – | – | Y | Y | – / elongation or filament |
| 1 | 5.6 | 97% | N | Y | |||
| 2 | 2.9 | 46% | N | N | |||
| MACSJ1423 | 0.5450 | 1 | 5.0 | 91% | Y | Y | Relaxed (1) |
| MACSJ1621 | 0.4650 | 1 | 6.8 | 97% | Y | Y | recent or present merger (3) / elongation or filament |
| 2 | 5.9 | 96% | N | Y | |||
| RXJ1716 | 0.8130 | 1 | 7.3 | 98% | Y | Y | past merger (2) |
| 2 | 4.9 | 85% | N | N | |||
| 3 | 5.4 | 86% | N | N | |||
| MS2053* | 0.5830 | 1 | 8.7 | 100% | Y | Y | past merger (2) |
| CXOSEXSI2056* | 0.6002 | 2 | 4.4 | 84% | Y | N | recent or present merger (3) |
| 3 | 4.5 | 84% | N | N | |||
| 4 | 3.2 | 55% | N | N | |||
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: structure ID; #4: significance of the WL peak in the 2D mass map in unit of σκ (see text for details); #5: percentage of redetection above 3σκ over the 100 noise realizations; #6: detection of the structure in X-rays (Y for yes, N for no, ~ when the detection is ambiguous, – for no data); #7: detection of the structure in galaxy density map (Y for yes, N for no, ~ when the detection is ambiguous, – for no data); and #8: derived status of the cluster from our analysis and possible presence of a large filament; numbers refer to the classification in the text.
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