Table 3.
CARLA selected overdensities.
| Selected cluster | zclus | Overdensity | Ngal | S/Nc | log |
log |
Est. field cont. | AGN |
|---|---|---|---|---|---|---|---|---|
| CARLAJ1358+5752 | 1.368 | 1 | 19 | 17 | 12.6 | 14.3 | 10% | C |
| CARLAJ1358+5752 | 1.368 | 2 | 18 | 15 | 11.2 | 13.8 | 10% | – |
| CARLAJ0958–2904 | 1.392 | 1 | 8 | 6 | 11.4 | 13.7 | 25% | C |
| CARLAJ0116–2052 | 1.425 | 1 | 18 | 16 | 11.7 | 14.0 | 10% | ∼0.5′ |
| CARLAJ1103+3449 | 1.442 | 1 | 12 | 10 | 11.5 | 13.6 | 15% | C |
| CARLAJ1131–2705 | 1.446 | 1 | 9 | 7 | 11.3 | 13.6 | 20% | C |
| CARLAJ2355–0002 | 1.490 | 1 | 17 | 15 | 11.7 | 14.0 | 10% | C |
| CARLAJ1129+0951 | 1.528 | 1 | 16 | 14 | 12.5 | 14.3 | 10% | ∼0.5′ |
| CARLAJ1753+6310 | 1.582 | 1 | 25 | 23 | 11.8 | 13.9 | 10% | C |
| CARLAJ1052+0806 | 1.646 | 1 | 17 | 15 | 12.0 | 14.1 | 10% | C |
| CARLAJ1300+4009 | 1.675 | 1 | 17 | 15 | 12.1 | 14.1 | 10% | C |
| CARLAJ2227–2705 | 1.692 | 0 | – | – | – | – | – | – |
| CARLAJ1510+5958 | 1.725 | 1 | 13 | 11 | 12 | 14.2 | 15% | C |
| CARLAJ1018+0530 | 1.952 | 1 | 13 | 11 | 11.9 | 14.0 | 15% | – |
| CARLAJ1018+0530 | 1.952 | 2 | 12 | 10 | 12.1 | 14.1 | 15% | C |
| CARLAJ0800+4029 | 1.986 | 1 | 19 | 17 | 12.3 | 14.3 | 10% | C |
| CARLAJ2039–2514 | 1.999 | 1 | 12 | 10 | 11.8 | 14.0 | 15% | C |
| CARLAJ2039–2514 | 1.999 | 2 | 10 | 8 | 11.6 | 13.6 | 20% | ∼0.7′ |
| CARLAJ1017+6116 | 2.801 | 1 | 16 | 14 | 12.6 | 14.6 | 10% | C |
Notes. We show the CARLA name of the cluster, the average cluster spectroscopic redshift ⟨zclus⟩ from Noirot et al. (2018), overdensity label (this is 0 if we did not select overdensities, 1 if we select only one overdensity, and 1 or 2 if we select two overdensities), the number of selected galaxies, the S/N in the selected circular region, the cluster total stellar mass, the approximate halo mass, the expected approximate percentage contamination of field galaxies in the selected circular region 
, and the position of the AGN: C indicates that the AGN is within ∼0.25′ from the overdensity peak; if it is not, we give the distance from the peak.
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