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Table 1

The sample of the five galaxy clusters used in this work.

Cluster name X-ray peak BCG NHa Redshift XMM exp.b Chandra exp.c w BCG X-ray peak
[J2000] [J2000] [1020 cm-3] [ks] [ks] [10-2R500] distance
M1 M2 PN ACIS XMM Chandra [10-2R500]

SPT-CLJ 2146-4632 21 46 34.78−46 32 54.06 21 46 34.57−46 32 57.20 1.64 0.933 147.5 157.4 102.2 70.9 2.49 ± 0.172.46 ± 0.78 7.04
PLCKG266.6-27.3d 06 15 51.83−57 46 46.58 06 15 51.77−57 46 48.61 4.32 0.972 11.4 12.4 2.9 226.7 0.68 ± 0.180.94 ± 0.11 1.62
SPT-CLJ 2341-5119 23 41 12.23−51 19 43.05 23 41 12.37−51 19 44.62 1.21 1.003 86.9 93.6 44.5 77.8 1.96 ± 0.162.98 ± 0.87 2.06
SPT-CLJ 0546-5345 05 46 37.22−53 45 34.43 05 46 37.63−53 45 30.49 6.79 1.066 126.0 127.9 112.9 67.9 1.16 ± 0.110.96 ± 0.34 5.63
SPT-CLJ 2106-5845 21 06 05.28−58 44 31.70 21 06 04.60−58 44 28.21 4.33 1.132 26.1 25.9 16.1 70.8 1.55 ± 0.211.90 ± 0.30 6.08

Notes.

(a)

The neutral hydrogen column density absorption along the line of sight is determined from the LAB survey (Kalberla et al. 2005).

(b,c)

We report the total exposure time after cleaning procedures.

(d)

SPT name: SPT-CLJ 0615-5746.

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