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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+3745b 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 J21464633 21 46 34.72 −46 32 50.86 0.933 1.64 80 90; 64 13469 0744400501
SPT-CL J23415119 23 41 12.23 −51 19 43.05 1.003 1.21 50 64; 34 11799 0744400401
SPT-CL J05465345 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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