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Table 1

XMM-Newton/EPIC observations used in this paper (see Pinto et al. 2015, for details on RGS observations).

Source ObsID Net exposure timea z b r500c Typed
MOS 1 MOS 2 pn
(ks) (ks) (ks) (Mpc)

2A 0335+096 0109870101 0147800201 85.7 86.6 81.4 0.0349 1.05 h
A 85 0723802101/2201 191.1 193.6 158.2 0.0556 1.21 h
A 133 0144310101 0723801301/2001 134.3 137.4 95.8 0.0569 0.94 h
A 189 0109860101 35.7 36.8 33.3 0.0318 0.50 c
A 262 0109980101 0504780201 53.4 54.7 43.2 0.0161 0.74 h
A 496 0135120201 0506260301/0401 131.4 138.2 103.3 0.0328 1.00 h
A 1795 0097820101 38.1 37.0 25.4 0.0616 1.22 h
A 1991 0145020101 29.2 29.3 20.5 0.0587 0.82 h
A 2029 0111270201 0551780201/0301/0401/0501 147.5 154.4 107.7 0.0767 1.33 h
A 2052 0109920101 0401520501/0801 93.0 92.7 53.7 0.0348 0.95 h
0401520901/1101/1201/1601
A 2199 0008030201/0301/0601 0723801101/1201 130.2 129.7 114.1 0.0302 1.00 h
A 2597 0147330101 0723801701 110.7 112.0 85.3 0.0852 1.11 h
A 2626 0083150201 0148310101 50.1 50.6 41.8 0.0573 0.84 h
A 3112 0105660101 0603050101/0201 186.6 190.8 153.6 0.0750 1.13 h
A 3526 / Centaurus 0046340101 0406200101 151.8 153.1 128.8 0.0103 0.83 h
A 3581 0205990101 0504780301/0401 113.0 117.8 84.1 0.0214 0.72 c
A 4038 / Klemola 44 0204460101 0723800801 78.7 79.6 71.4 0.0283 0.89 h
A 4059 0109950101/0201 0723800901/1001 194.9 198.5 153.9 0.0460 0.96 h
AS 1101 / Sérsic 159-03 0123900101 0147800101 121.0 122.9 108.8 0.0580 0.98 h
AWM 7 0135950101 0605510101 148.7 149.6 153.9 0.0172 0.86 h
EXO 0422 0300210401 39.5 38.9 34.9 0.0390 0.89 h
Fornax / NGC 1399 0012830101 0400620101 106.2 114.2 75.1 0.0046 0.40 c
HCG 62 0504780501/0601 121.8 126.7 101.6 0.0146 0.46 c
Hydra A 0109980301 0504260101 96.3 101.5 74.7 0.0538 1.07 h
M 49 / NGC 4472 0112550601 0200130101 93.1 94.8 86.3 0.0044 0.53 c
M 60 / NGC 4649 0021540201 0502160101 118.4 119.1 108.0 0.0037 0.53 c
M 84 / NGC 4374 0673310101 32.0 34.0 30.5 0.0034 0.46 c
M 86 / NGC 4406 0108260201 68.4 70.4 47.0 -0.0009 0.49 c
M 87 / NGC 4486 0114120101 0200920101 113.9 114.5 96.8 0.0044 0.75 c
M 89 / NGC 4552 0141570101 23.2 24.4 18.3 0.0010 0.44 c
MKW 3s 0109930101 0723801501 147.7 148.9 126.9 0.0450 0.95 h
MKW 4 0093060101 0723800701 75.5 74.9 56.9 0.0200 0.62 h
NGC 507 0080540101 0723800301 124.4 124.8 103.7 0.0165 0.60 c
NGC 1316 / Fornax A 0302780101 0502070201 123.7 127.2 75.2 0.0059 0.46 c
NGC 1404 0304940101 26.8 14.8 21.0 0.0064 0.61 c
NGC 1550 0152150101 0723800401/0501 166.3 167.0 128.2 0.0123 0.62 c
NGC 3411 0146510301 21.4 21.6 19.8 0.0155 0.47 c
NGC 4261 0056340101 0502120101 108.6 109.8 85.8 0.0074 0.45 c
NGC 4325 0108860101 20.2 19.0 16.3 0.0258 0.58 c
NGC 4636 0111190701 56.1 56.3 54.5 0.0037 0.35 c
NGC 5044 0037950101 0554680101 119.0 121.8 100.4 0.0090 0.56 c
NGC 5813 0302460101 0554680201/0301 138.2 143.2 106.8 0.0064 0.44 c
NGC 5846 0021540501 0723800101/0201 171.0 173.9 147.9 0.0061 0.36 c
Perseus 0085110101 0305780101 155.5 156.6 132.1 0.0183 1.29 h

Total 4 492.3 4 563.6 3 666.9

Notes. The new observations from the CHEERS proposal are shown in boldface.

(a)

Total exposure time after cleaning the data from soft flares (see text).

(b)

Redshifts were taken from Reiprich & Böhringer (2002), except for A 189 (Hudson et al. 2001); A 1991, A 2626, HCG 62, and M 87 (ACCEPT catalog Cavagnolo et al. 2009); M 89 (Mahdavi & Geller 2001); NGC 1316 (Pinto et al. 2014); NGC 1404 (Morris et al. 2007); M 84, M 86, NGC 4261, and NGC 4649 (Smith et al. 2000).

(c)

Values of r500 were taken from Pinto et al. (2015, and references therein).

(d)

Classification of the objects. The letter h stands for the “hot” clusters (>1.7 keV), while the letter c stands for the “cool” groups/ellipticals (<1.7 keV). M 87 is an exception, and is classified as cool even though its central temperature is about ~2 keV (see text).

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