Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS

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Volume 585 (January 2016)

A&A, 585 (2016) A130

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201526925e]

Table A.3

Chandra cluster sample (REFLEX clusters).

Cluster^a	Exp.^b	RA (J2000)	Dec (J2000)	Flux^c	z	Obj. ID (REFLEX)	L _X ^d
	[ks]	[deg]	[deg]	[10^-15 W/m²]			[10³⁷ W]

SERSIC 159-03	106	348.515	−42.713	23.412	0.0564	J2313.9−4244	3.74
A 496	88	68.403	−13.25	72.075	0.0326	J0433.6−1315	3.89
HYDRA A	224	139.527	−12.092	39.461	0.0539	J0918.1−1205	5.61
A 1650	229	194.664	−1.781	20.909	0.0845	J1258.6−0145	6.99
A 2597	146	351.337	−12.136	20.558	0.0852	J2325.3−1207	7.22
A 3667	528	303.211	−56.855	70.892	0.0556	J2012.5−5649	10.02
A 907	103	149.528	−11.086	7.833	0.1669	J0958.3−1103	10.13
A 521	165	73.558	−10.273	4.944	0.2475	J0454.1−1014	12.97
A 2744	124	3.586	−30.352	4.964	0.3066	J0014.3−3023	19.79
A 1689	197	197.808	−1.337	15.332	0.1832	J1311.4−0120	23.59
1E 0657-56	566	104.751	−55.904	9.079	0.2965	J0658.5−5556	35.55
RX J1347-114	232	206.889	−11.734	6.468	0.4516	J1347.5−1144	63.43

Notes.

^(a)

Most commonly used name of cluster or central object.

^(b)

Combined ACIS-S/-I exposure after excluding times of high background.

^(c)

ROSAT 0.1−2.4 keV X-ray flux in 10^-15 W/m².

^(d)

ROSAT 0.1−2.4 keV X-ray luminosity in 10³⁷ W (REFLEX column: LumCor, h = 0.5).

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