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Table 1

XMM-Newton RGS data of the sample clusters.

Cluster Observation ID Total clean time (ks) kT(a) (keV) z O abundance
2A 0335+096 0109870101 0147800201 91.6 4.0 0.0349 0.59
A85 0723802101/2201 155.6 6.1 0.0557 0.55
A133 0144310101 0723801301/2001 136.0 3.8 0.0569 0.67
A262 0109980101 0504780201 80.3 2.2 0.0161 0.56
A383 0084230501 22.3 3.1 0.1871 0.38
A496 0095010901 0135120201/0801 0506260301/0401 152.4 4.1 0.0328 0.60
A1795 0097820101 31.8 6.0 0.0616 0.35
A1991 0145020101 37.8 2.7 0.0586 0.65
A2029 0111270201 0551780201/0301/0401/0501 156.7 8.7 0.0767 0.41
A2052 0109920101/0201/0301 0401520301/0501/0601 153.5 3.0 0.0348 0.52
0401520801/0901/1101/1201/1301/1601/1701
A2199 0008030201/0301/0601 0723801101/1201 118.6 4.1 0.0302 0.62
A2204 0112230301 0306490101/0201/0301/0401 77.0 5.6 0.1511 0.28
A2597 0147330101 0723801601/1701 175.8 3.6 0.0852 0.54
A3112 0105660101 0603050101/0201 162.2 4.7 0.0750 0.51
A3581 0205990101 0504780301/0401 119.8 1.8 0.0214 0.47
A4038 0204460101 0723800801 67.1 3.2 0.0283 0.66
A4059 0109950101/0201 0723800901/1001 200.7 4.1 0.0460 0.58
AS 1101 0123900101 0147800101 124.2 3.0 0.0580 0.32
EXO 0422 0300210401 29.6 3.0 0.0390 0.65
Hydra-A 0109980301/0501 0504260101 118.0 3.8 0.0538 0.35
ZW 3146 0108670101 0605540201/0301 166.2 3.6 0.2906 0.45

Temperatures, redshifts, and oxygen abundances are taken from de Plaa et al. (2017), except for Abell 383, Abell 2204, and ZW 3146. The best-fit values obtained with single-temperature modeling (Sect. 5) are given for these three objects.

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