Table 1.
CARLA confirmed cluster sample.
| Name | zAGN | zclus | Other name | Nspec | σdet | 1+δspec | AGN type | Classification |
|---|---|---|---|---|---|---|---|---|
| CARLAJ1358+5752 | 1.370 | 1.368 | J1358+5752 | 14 | 19.4 | 6.8 | RLQ | PC |
| CARLAJ0958–2904 | 1.411 | 1.392 | MRC0955–288 | 8 | 19 | 3.5 | HzRG | PC |
| CARLAJ0116–2052 | 1.417 | 1.425 | MRC0114–211 | 12 | 18 | 6.3 | HzRG | PC |
| CARLAJ1103+3449 | 1.444 | 1.442 | 6CE1100+3505 | 8 | 21.0 | 3.9 | HzRG | PC |
| CARLAJ1131–2705 | 1.444 | 1.446 | MRC1128–268 | 9 | 17.8 | 5.1 | HzRG | PC |
| CARLAJ2355–0002 | 1.487 | 1.490 | TXS2353–003 | 12 | 19.4 | 6.3 | HzRG | PC |
| CARLAJ1129+0951 | 1.520 | 1.528 | J1129+0951 | 12 | 21.0 | 6.3 | RLQ | PC |
| CARLAJ1753+6310 | 1.576 | 1.582 | 7C1753+6311 | 5 | 17.5 | 2.8 | HzRG | HPC |
| CARLAJ1052+0806 | 1.641 | 1.646 | J1052+0806 | 6 | 19 | 6.2 | RLQ | PC |
| CARLAJ2227–2705 | 1.684 | 1.692 | MRC2224–273 | 7 | 18.5 | 6.2 | HzRG | PC |
| CARLAJ1300+4009 | 1.669 | 1.675 | J1300+4009 | 8 | 18.1 | 7.2 | RLQ | PC |
| CARLAJ1510+5958 | 1.719 | 1.725 | J1510+5958 | 6 | 19.4 | 6.2 | RLQ | PC |
| CARLAJ1018+0530 | 1.949 | 1.952 | J1018+0530 | 8 | 18 | 8.6 | RLQ | PC |
| CARLAJ2039–2514 | 1.997 | 1.999 | MRC2036–254 | 9 | 22.6 | 9.8 | HzRG | HPC |
| CARLAJ0800+4029 | 2.004 | 1.986 | J0800+4029 | 10 | 21 | 11.0 | RLQ | PC |
| CARLAJ1017+6116 | 2.80 | 2.801 | J1017+6116 | 7 | 21 | 47.9 | RLQ | HPC |
Notes. From Noirot et al. (2018; Tables 2 and 4) and Wylezalek et al. (2014): the CARLA name of the cluster, the AGN redshift zAGN, the average cluster spectroscopic redshift zclus, other names for the cluster (when this applies), the number of spectroscopically confirmed members Nspec, the significance of the detection from the Spitzer colour selection σdet from Wylezalek et al. (2014), the significance of the spectroscopic selection HST (1+δspec), the AGN type, and the cluster classification. HzRG labels high redshift radio galaxies, and RLQ labels radio loud quasars. HPC and PC indicate a ‘highly probable confirmed cluster’ and ‘probable confirmed cluster’, respectively, as defined in Noirot et al. (2018).
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