Clusters of Galaxies in a Weyl Geometric Approach to Gravity

Table 2

Dataset used for halo model (error intervals omitted).

Cluster
Coma	0.654	246	1.278	6.55	8.42	13.14	13.84	2.3	12.86
A85	0.532	59.3	1.216	6.37	8.13	7.36	7.71	1.9	8.72
A400	0.534	110.	0.712	1.83	1.36	4.39	1.48	1.09	2.93
IIIZw54	0.887	206	0.731	1.91	1.45	4.57	2.81	1.35	4.51
A1367	0.695	274	0.893	1.76	2.07	4.35	4.06	1.53	5.77
MKW4	0.44	7.86	0.58	0.5	0.47	1.16	0.71	0.86	1.79
ZwCl215	0.819	308	1.098	4.93	6.1	7.05	10.37	2.09	10.65
A1650	0.704	201	1.087	3.44	5.09	7.47	11.14	2.15	11.11
A1795	0.596	55.7	1.118	3.41	5.11	6.21	10.99	2.14	11.04
MKW8	0.511	76.4	0.715	0.62	0.8	1.61	2.38	1.28	4.0
A2029	0.582	59.3	1.275	14.7	13.35	9.59	13.42	2.29	12.59
A2052	0.526	26.4	0.875	1.39	1.86	3.53	2.21	1.25	3.79
MKW3S	0.581	47	0.905	1.45	2.13	3.9	3.46	1.45	5.11
A2065	1.162	493	1.008	11.18	7.66	7.32	16.69	2.45	14.46
A2142	0.591	110	1.449	7.36	13.76	8.42	15.03	2.36	13.61
A2147	0.444	170.	1.064	4.44	5.04	6.84	3.46	1.45	5.15
A2199	0.655	99.2	0.957	2.69	2.97	4.76	4.80	1.62	6.37
A2255	0.797	423	1.072	7.13	7.11	6.74	13.32	2.27	12.52
A2589	0.596	84.3	0.848	3.03	2.54	5.12	3.58	1.47	5.24

Source: , , , , and from [15]; from [3]; , , and from [2].
Units. in kpc, , in Mpc, in  , in  , and in  .