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Table 5.
CARLA-selected spectroscopically confirmed member classification as passive and active galaxies in this paper.
| Cluster | ID | Tile | z | log(sSFR) | SFR flux | Classification |
|---|---|---|---|---|---|---|
| CARLA J0800+4029 | 436 | t1-1523 | 1.969±0.007 | −9.4±0.5 | OIII | Passive |
| CARLA J1129+0951 | 240 | t1-1222 | 1.546±0.004 | −8.7±0.5 | Hα | Active |
| CARLA J1129+0951 | 261 | t1-1263 | 1.537±0.006 | −9.1±0.5 | Hα | Passive |
| CARLA J1358+5752 | 414 | t1-1462 | 1.377±0.006 | −8.9±0.5 | Hα | Active |
| CARLA J1358+5752 | 681 | t1-1794 | 1.376±0.005 | −9.4±0.5 | Hα | Passive |
| CARLA J1358+5752 | 694 | t1-1795 | 1.375±0.006 | −9.3±0.5 | Hα | Active |
| CARLA J2355–0002 | 762 | t1-1374 | 1.492±0.005 | −9.2±0.6 | Hα | Passive |
| CARLA J2355–0002 | 334 | t1-1405 | 1.485±0.007 | −9.1±0.5 | Hα | Passive |
| CARLA J2355–0002 | 337 | t1-1410 | 1.500±0.006 | −9.6±0.3 | Hα | Passive |
| CARLA J2039–2514 | 174 | t1-1236 | 2.000±0.007 | −8.4±0.5 | OIII | Active |
Notes. We include only the spectroscopically confirmed members included in the galaxy selection used in this paper. In the column SFR flux, we show which line emission flux was used to estimate the SFR.
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