Open Access
Table 1.
Studies from which ram pressure stripped candidates are sourced in this study.
| Study | Cluster | Detection method | No. of RPS candidates with GZ2 data |
|---|---|---|---|
| (instrument) | (total including doubles) | ||
| Gavazzi et al. (1984) | Abell 1367 | 1.4 GHz (VLA) | 1 |
| Conselice & Gallagher (1998) | Coma | Optical (WIYN) | 1 |
| Yagi et al. (2007) | Coma | Hα (Suprime-Cam) | 1 |
| Smith et al. (2010) | Coma | UV (Galex) | 6 (10) |
| Yagi et al. (2010) | Coma | Hα (Suprime-Cam) | 10 (13) |
| Kenney et al. (2015) | Coma | Optical (Hubble) | 1 |
| Poggianti et al. (2016) | Wings Clusters | Optical (WINGS) | 37 |
| Poggianti et al. (2016) | PM2GC Groups | Optical (MGC) | 24 |
| Gavazzi et al. (2017) | Abell 1367 | Hα (Suprime-Cam) | 1 |
| Roberts & Parker (2020) | Coma | Optical (CFHT) | 20 (41) |
| Roberts et al. (2021b) | Various clusters | 144 MHz (LOFAR) | 63 (66) |
| Roberts et al. (2021a) | Various groups | 144 MHz (LOFAR) | 47 |
Notes. The values in the final column denote how many galaxies have corresponding Galaxy Zoo 2 data. The values in brackets indicate the number of galaxies, including duplicates, where a galaxy is present in multiple studies.
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