Table 2: Observation log.
Cluster XMM Exposure time (ks)a $H_{\rm t}$b Average Hc moded filtere
name orbit MOS1 MOS2 pn MOS pn MOS1 MOS2 pn pn  
NGC 533 195 38 38 31 35 50 21.8 22.3 28.9 FF thin
Virgo 97 34 33 25 35 50 25.6 26.2 36.8 FF thin
A 262 203 24 24 15 35 50 25.1 24.6 33.0 FF thin
A 1837 200 48 48 40 35 50 21.5 22.3 29.7 EFF thin
Sérsic 159-3 77 31 32 28 35 50 25.5 24.7 32.5 FF thin
MKW 9 311 22 23 13 35 50 27.9 28.4 31.1 EFF thin
2A 0335+096 215 11 11 5 50 56 28.4 29.5 27.2 FF thin
MKW 3s 129 37 37 32 35 50 22.1 22.5 31.2 FF thin
A 2052 128 30 30 23 35 50 21.4 21.7 29.6 EFF thin
A 4059 176 13 13 6 50 56 33.2 32.3 34.1 FF thin
  176 21 20 - 40 - 28.2 28.8 - FF thin
Hydra A (A 780) 183 17 17 3 50 56 32.8 32.4 31.6 FF thin
A 496 211 9 10 5 35 56 27.3 25.6 38.9 EFF thin
A 3112 191 22 22 16 35 50 24.7 24.3 34.4 EFF med
A 1795 100 29 30 22 35 52 25.9 25.8 38.8 FF thin
A 399 127 13 13 6 35 50 22.2 23.9 31.3 EFF thin
A 3266 153 24 24 19 35 50 24.0 21.7 28.9 EFF med
Perseus (A 426) 210 43 46 33 80 120 62.5 64.9 82.5 FF thin
Coma (A 1656) 86 15 16 13 35 50 24.7 24.9 42.9 FF med
A 754 262 14 14 11 35 50 24.2 24.6 34.4 EFF med
A 1835 101 - 26 25 35 50 - 24.2 33.4 FF thin
Background - 410 379 324 60 50 23.8 23.1 30.8 FF thin
a Net exposure time, after rejection of soft proton flares.
b Background rejection threshold for soft proton flares, in counts per 260 s between 10-12 keV.
c Average background after rejection of soft proton flares, in counts per 260 s between 10-12 keV.
d Mode pn: extended full frame (EFF) of full frame (FF).
e Filter used for MOS and pn.
f Number of rejected point sources.

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