Table 1.
General properties of the clusters investigated in this study.
| ID | RA | Dec | z | M200 | R200 | σ | References |
|---|---|---|---|---|---|---|---|
| (hh:mm:ss) | (dd:mm:ss) | (1014 M⊙) | (Mpc) | (km s−1) | |||
| Abell 901/902 | – | – | – | – | – | – | – |
| A901a | 09:56:27 | −09:57:22 | 0.16 | 1.3 ± 0.3 | 0.8 ± 0.1 | 880 ± 30 | |
| A901b | 09:55:57 | −09:59:03 | 0.16 | 1.3 ± 0.3 | 0.8 ± 0.1 | 940 ± 20 | Heymans et al. (2008) |
| A902 | 09:56:34 | −10:10:00 | 0.17 | 0.4 ± 0.2 | 0.6 ± 0.1 | 810 ± 20 | Weinzirl et al. (2017) |
| SW Group | 09:55:39 | −10:10:19 | 0.17 | 0.6 ± 0.2 | 0.6 ± 0.1 | 590 ± 40 | |
| RXJ 1347 | – | – | – | – | – | – | – |
| RXJ 1347-1145 | 13:47:31 | −11:45:10 | 0.45 | 11.6 ± 3.0 | 1.9 ± 0.2 | 1160 ± 100 | Lu et al. (2010) |
| RXJ 1347-1145 | 13:46:27 | −11:54:28 | 0.47 | 5.6 ± 1.6 | 1.2 ± 0.2 | 780 ± 100 | |
| CL1604 | – | – | – | – | – | – | – |
| CL1604+4304 | 16:04:22 | 43:04:56 | 0.90 | 3.3 ± 1.5 | 0.9 ± 0.2 | 720 ± 130 | Lemaux et al. (2012), |
| CL1604+4321 | 16:04:34 | 43:21:14 | 0.92 | 1.8 ± 1.6 | 0.8 ± 0.1 | 690 ± 90 | Wu et al. (2014) |
| XMMU J2235.3-2557 | 22:35:21 | 25:57:40 | 1.39 | 7.3 ± 1.3 | 1.1 ± 0.1 | 1180 ± 90 | Jee et al. (2009) |
| HSC-CL2329 | 23:30:05 | 00:12:36 | 1.47 | – (a) | – | < 400 | Böhm et al. (2020) |
| HSC-CL2330 | 23:30:22 | −00:24:00 | 1.47 | – (a) | – | < 400 | Böhm et al. (2020) |
Notes. The table lists: IDs, right ascension, declination, redshift, virial mass (M200) and size (R200), velocity dispersion, and references for these measurements.
These two protoclusters are most probably not yet virialized structures. Thus, no velocity dispersion-based mass can be computed. See Böhm et al. (2020) for more details.
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