The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319

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Table B.1

Statistical results of the fitting in the annular regions.

Radii	C-stat.	PHA bins	C-stat. reduced	Net cts	SBR	n_H
arcmin	–	–	–	10³	–	10²² cm⁻²
0.00–1.05	2746	2603	1.05	170	85	0.075
1.05–1.63	2698	2591	1.04	155	58	0.078
1.63–2.18	2748	2552	1.08	148	42	0.081
2.18–2.74	2773	2575	1.08	145	32	0.077
2.74–3.32	2767	2484	1.11	131	24	0.078
3.32–3.98	2688	2573	1.05	133	17	0.081
3.98–4.65	2807	2582	1.09	134	14	0.079
4.65–5.37	2912	4005	0.73	131	11	0.075
5.37–6.14	2666	2387	1.13	112	8.6	0.074
6.14–6.95	2811	2481	1.13	101	6.8	0.077
6.95–7.83	3157	4949	0.64	92	5.1	0.074
7.83–8.85	3305	3866	0.85	89	3.6	0.073
8.85–10.05	3697	6052	0.61	82	2.5	0.074
10.05–11.51	4514	3868	1.17	80	1.7	0.076
11.51–13.10	4870	3583	1.36	62	1.2	0.079
13.10–15.18	4893	3494	1.40	46	0.9	0.077
15.18–17.70	2808	1844	1.52	20	0.9	0.121
17.70–20.63	2632	2175	1.21	19	0.6	0.101
20.63–24.08	2098	1916	1.09	12	0.4	0.113

Notes. Thetable lists: radial extension, C-statistic, number of spectral bins, reduced C-statistic indicated, net number of photons in the energy band [0.5–11.3] keV, signal-to-background ratio, and best-fit n_H.

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