Searching for rotation in X-COP galaxy clusters | Astronomy & Astrophysics (A&A)

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Table 1.

Priors on M₂₀₀ and lnc₂₀₀ of our models.

Cluster	z	M₂₀₀^median	σ_M	$ln c_{200}^{median}$ $\ln c_{200}^{\mathrm{median}}$
A85	0.0555	0.84	0.27	1.22
A644	0.0704	0.83	0.25	1.24
A1644	0.0473	0.66	0.20	1.24
A1795	0.0622	1.39	0.28	1.19
A2142	0.090	1.45	0.30	1.19
A2255	0.0809	1.07	0.32	1.21
A2319	0.0557	2.01	0.59	1.17
A3158	0.0597	0.73	0.22	1.23
A3266	0.0589	1.45	0.49	1.19
RXC1825	0.0650	0.69	0.20	1.24
Zw1215	0.0767	0.51	0.27	1.26

Notes. Columns: cluster name, redshift, median and standard deviation of the normal prior on M₂₀₀, median of the prior on lnc₂₀₀. The standard deviation of lnc₂₀₀ is 0.38 for all the clusters. M₂₀₀^median and σ_M are in units of 10¹⁵ M_⊙.

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