Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra

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Volume 608 (December 2017)

A&A, 608 (2017) A88

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Table 1

Observational properties of the 12 clusters used in this work.

Cluster name	RA	Dec	z	N _H ^a	Chandra	XMM-Newton	Chandra	XMM-Newton
					exp.	exp. (MOS1,2; PN)	obs. ID	obs. ID
	[J2000]	[J2000]		[ 10²⁰ cm ^-3 ]	[ ks]	[ ks]

A1651	12 59 22.15	−04 11 48.24	0.084	1.81	10	7; 5	4185	0203020101
A1650	12 58 41.48	−01 45 40.45	0.084	0.72	37	34; 30	7242	0093200101
A1413	11 55 17.97	+ 23 24 21.99	0.143	1.84 ^*	75	63; 52	5003	0502690201
A2204	16 32 46.94	+ 05 34 32.63	0.152	6.97 ^*	77	14; 10	7940	0306490201
A2163	16 15 46.06	−06 08 52.36	0.203	16.50 ^*	71	92; 65^†	1653	0694500101
A2390	21 53 36.82	+ 17 41 43.30	0.231	8.66	95	10; 8	4193 ^•	0111270101
MACS J1423.8+2404	14 23 47.92	+ 24 04 42.96	0.545	2.20	115	34; 22^†	4195 ^•	0720700301
MACS J0717.5+3745^b	07 17 31.75	+ 37 45 31.02	0.546	6.64	58	59; 52	16305	0672420201
MACS J0744.9+3927	07 44 52.78	+ 39 27 26.63	0.698	5.66	50	52; 42^†	6111	0551851201
SPT-CL J2146−4633	21 46 34.72	−46 32 50.86	0.933	1.64	80	90; 64^†	13469	0744400501
SPT-CL J2341−5119	23 41 12.23	−51 19 43.05	1.003	1.21	50	64; 34^†	11799	0744400401
SPT-CL J0546−5345	05 46 37.22	−53 45 34.43	1.066	6.77	27	45; 33^†	9336	0744400201

Notes. The coordinates indicate the position of the X-ray peak used as the centre for profile extraction. The peak was determined using Chandra observations in the [0.7−2.5] keV band. .

^(a)

The neutral hydrogen column density was derived from the LAB survey (Kalberla et al. 2005).

^(b)

The X-ray peak is centred on the main structure, identified as region “B” in Limousin et al. (2016).

^(*)

The absorption value was estimated in a region which maximises the S/N

^(†)

MOS 2 effective exposure times are 3−4% higher than MOS1, except for MACS J1423.8+2404, for which the MOS2 exposure time is 43 ks.

^(•)

ACIS-S observations.

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