Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data

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Table 4.

Cluster properties.

Name	RA_cluster, X	Dec_cluster, X	Ref	M_200, c	Method	Ref	PA_cluster	Ref
	(J2000)	(J2000)		10¹⁴ M_⊙			(degrees)
SPT-CLJ0000–5748	0.25	−57.8093	1	6.04	SZ	1	170 ± 22	2
Cl0016+1609				25.76	WL	3	35 ± 0	4
SpARCS–J0035	8.9588	−43.2029	5	2.5	σ − M₂₀₀	6	154 ± 8	2
ACO2813	10.8519	−20.6229	7	8.17	WL	8
XDCPJ0044–2033	11.022	−20.5665	9	3.98	X	10	128 ± 49	2
RXJ0056–27	14.2338	−27.67	11	2.84	WL	3
SPT-CLJ0102–4915	15.734	−49.2656	1	25.4	WL	3	147 ± 2	2
RXJ0110+19	17.575	19.6397	11	2.36	WL	3
Abell209	22.969	−13.6108	12	9.5	Lens	13	131 ± 0	4
CLJ0152–1357	28.1712	−13.9686	14	14.0	WL	15
...	...	...	...	...	...	...	...	...

Notes. The columns are: full cluster name, X-ray coordinates of the cluster, mass of the cluster, method used to measure the mass of the cluster, PA of the cluster. The full table is available at the CDS.

References. (1) Chiu et al. (2015); (2) West et al. (2017); (3) Sereno (2015); (4) Durret et al. (2019); (5) Fassbender et al. (2011); (6) van der Burg et al. (2014); (7) Bartalucci et al. (2019); (8) Okabe & Smith (2016); (9) Tozzi et al. (2015); (10) Cooke et al. (2019b); (11) Hoekstra et al. (2010); (12) Postman et al. (2012b); (13) Merten et al. (2015); (14) Sayers et al. (2019); (15) Martinet et al. (2016); (16) DeMaio et al. (2019); (17) Jee et al. (2011); (18) Andreon et al. (2014); (19) Zitrin et al. (2012); (20) Stott et al. (2010); (21) Czakon et al. (2015); (22) Herbonnet et al. (2020); (23) Sereno & Zitrin (2011); (24) Brodwin et al. (2015); (25) Chan et al. (2019); (26) Jee et al. (2005); (27) Hicks et al. (2013); (28) Just et al. (2019); (29) Hicks et al. (2008); (30) Noble et al. (2011); (31) Gonzalez et al. (2015); (32) Dahle (2006); (33) Guennou et al. (2014); (34) Jørgensen et al. (2018); (35) Santos et al. (2012); (36) Jee et al. (2017); (37) Mo et al. (2016); (38) Martini et al. (2013); (39) Richard-Laferrière et al. (2020); (40) Sereno & Covone (2013); (41) Lidman et al. (2012); (42) Sanders et al. (2017); (43) Donnarumma et al. (2009).

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