Table 1.
Summary of the sample of galaxy clusters used in this paper.
| Cluster name | RA (J2000) | Dec. (J2000) | Redshift z | Mass M200 |
|---|---|---|---|---|
| (1014 M⊙) | ||||
| Perseus (NGC 1275) | 03h19m48.16s | 41d30m42.11s | 0.018 |  (1) |
| Abell 1795 | 13h49m00.50s | 26d35m07.00s | 0.063 |  (2) |
| v Abell 2029 | 15h10m58.70s | 05d45m42.00s | 0.077 | 11.2 ± 0.4 (3) |
| ZwCl 2701 | 09h52m49.10s | 51d53m05.00s | 0.214 | 5.2 ± 0.5 (3) |
| 4C+55.16 | 08h34m54.90s | 55d34m21.07s | 0.241 | 0.923 ± 0.182 (4) |
| RX J1532.9+3021 | 15h32m53.78s | 30d20m59.41s | 0.363 | 11.1 ± 1.1 (3) |
| MACS J1720.2+3536 | 17h20m16.80s | 35d36m27.00s | 0.391 | 8.1 ± 1.3 (3) |
| MACS J1423.8+2404 | 14h23m47.70s | 24d04m40.00s | 0.545 | 7.2 ± 0.9 (3) |
| Perseus (NGC 1275) | 03h19m48.16s | 41d30m42.11s | 0.018 |  (1) |
| Abell 2199 | 16h28m37.00s | 39d31m28.00s | 0.030 |  (5,6) |
| 2A 0335+096 | 03h38m35.30s | 09d57m54.00s | 0.035 |  (5,7) |
| MKW 3S | 15h21m50.70s | 07d42m18.00s | 0.045 | 5.1 (8) |
| Abell 1668 | 13h03m44.90s | 19d16m37.20s | 0.064 | 4.31 ± 1.63 (9) |
| Abell 2029 | 15h10m58.70s | 05d45m42.00s | 0.077 | 11.2 ± 0.4 (3) |
| 3C 388 | 18h44m02.42s | 45d33m29.81s | 0.092 | ... |
| MS 0735.6+7421 | 07h41m40.30s | 74d14m58.00s | 0.216 | 7.12 ± 1.96 (10) |
Notes. The horizontal line separates the clusters that are studied at high resolutions (∼ 0.3 arcsec, top half) from the clusters that are studied at low resolutions (∼ 6 arcsec, bottom half).
References. (1) Simionescu et al. (2011); (2) Reiprich & Böhringer (2002); (3) Mantz et al. (2016); (4) Takey et al. (2011); (5) Comerford & Natarajan (2007); (6) Łokas et al. (2006); (7) Voigt & Fabian (2006); (8) Pinzke et al. (2011); (9) Kopylova & Kopylov (2017); (10) Gitti et al. (2007).
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