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 B.1

Chandra datasets used in this study.

Cluster^a	Chandra ObsID^b

1e0657	554, 3184, 4984, 4985, 4986, 5355, 5356, 5357, 5358, 5361
2a0335	919, 7939, 9792
3c348	1625, 5796, 6257
a1413	537, 1661, 5002, 5003, 7696
a1650	4178, 5822, 5823, 6356, 6357, 6358, 7242, 7691
a1689	540, 1663, 5004, 6930, 7289, 7701
a1775	12891, 13510
a1795	493, 494, 3666, 5286, 5287, 5288, 5289, 5290, 6159, 6160, 6161, 6162, 6163,
	10432, 10433, 10898, 10899, 10900, 10901, 12026, 12027, 12028, 12029, 13106, 13107,
	13108, 13109, 13110, 13111, 13112, 13113, 13412, 13413, 13414, 13415, 13416, 13417,
	14268, 14269, 14270, 14271, 14272, 14273, 14274, 14275, 15485, 15486, 15487, 15488, 15489,
	15490, 15491, 15492, 16432, 16433, 16434, 16435, 16436, 16437, 16438, 16439, 16465, 16466,
	16467, 16468, 16469, 16470, 16471, 16472
a1835	495, 496, 6880, 6881, 7370
a1995	906, 7021, 7713
a2034	2204, 7695, 12885, 12886, 13192, 13193
a2052	890, 5807, 10477, 10478, 10479, 10480, 10879, 10914, 10915, 10916, 10917
a2146	10464, 10888, 12245, 12246, 12247, 13020, 13021, 13023, 13120, 13138
a2199	497, 498, 10748, 10803, 10804, 10805
a2204	499, 6104, 7940
a2390	500, 501, 4193
a2597	922, 6934, 7329, 15144
a2744	2212, 7712, 7915, 8477, 8557
a3667	513, 889, 5751, 5752, 5753, 6292, 6295, 6296, 7686
a401	518, 2309, 14024
a496	931, 3361, 4976
a520	528, 4215, 7703, 9424, 9425, 9426, 9430
a521	430, 901, 12880, 13190
a665	531, 3586, 7700, 12286, 13201, 15148
a907	535, 3185, 3205
cygnusa	360, 5830, 5831, 6225, 6226, 6228, 6229, 6250, 6252
hydraa	575, 576, 4969, 4970
ms0735	4197, 10468, 10469, 10470, 10471, 10822, 10918, 10922
ms1455	543, 4192, 7709
pks0745	508, 2427, 6103, 7694, 12881
rxj1347	506, 507, 3592, 13516, 13999, 14407
sersic159	1668, 11758
zw3146	909, 9371

Notes.

^(a)

Abbreviated cluster name.

^(b)

List of Chandra observations used in this study (indicated by their ObsID, observation identification number).

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