Table 1.
Redshift range, cluster mass range, AGN luminosity LX (or flux FX) of the AGNs, and magnitudes of optically selected galaxies from several studies, shown in Fig. 12.
| Study | z range | M500 (M⊙) | AGN X-ray selection | Galaxy selection |
|---|---|---|---|---|
| Koulouridis 2019 | 0.93–1.13 | 5 × 1014 − 9 × 1014 | LX(0.5 − 8 keV) > 3 × 1042 erg s−1 | R < 23, SuprimeCam R-band, M* ≳ 1010 M⊙ |
| Koulouridis 2018 | 0.1–0.5 | 1013 − 5 × 1014 | LX(0.5 − 10 keV) > 1042 erg s−1 |  |
| Ehlert 2014 | 0.2–0.7 | 4.7 × 1014 − 2.2 × 1015 | FX(0.5 − 8.0 keV) > 10−14 erg cm−2 s−1 | R < 23, SuprimeCam R-band, M* ≳ 1010 M⊙ |
| Haines 2012 | 0.15–0.3 | ≳5 × 1014 | LX(0.3 − 7 keV)≳1042 erg s−1 | Mk < −23.1 |
| Koulouridis 2010 | 0.07–0.28 | LX(0.5 − 8 keV) > 1042 erg s−1 |
 |
|
| Martini 2007 | 0.06–0.31 | LX > 1042 erg s−1 and LX > 1041 erg s−1 | MR < −20 |
Notes. We refer the reader to original papers and references therein for descriptions of the magnitude thresholds R, 
, Mk, and mr, and details about the selected clusters where their mass is not given explicitly.
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