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| Cluster | Obs ID | za | NHb | Exp.timec |
 d
|
||
| 1022 cm-2 | MOS1 | MOS2 | pn | arcmin (kpc) | |||
| Abell 85 | 0065140101 | 0.0551 | 0.0342 | 12.5 | 12.5 | 9.7 | 1.137 (73) |
| Abell 262 | 0109980101 | 0.0163 | 0.0538 | 23.8 | 23.9 | 19.2 | 2.613 (52) |
| AWM7 | 0135950301 | 0.0172 | 0.0983 | 30.7 | 30.7 | 28.7 | 2.473 (52) |
| Abell 3112 | 0105660101 | 0.0750 | 0.0261 | 23.3 | 23.3 | 18.6 | 1.124 (96) |
| Perseus | 0085110101 | 0.0179 | 0.1410 | 53.7 | 53.7 | 51.3 | 4.263 (93) |
| 2A 0335+096 | 0147800201 | 0.0349 | 0.1780 | 80.2 | 80.9 | 73.9 | 2.596 (108) |
| Abell 478 | 0109880101 | 0.0881 | 0.1510 | 28.7 | 79.0 | 42.6 | 1.032 (102) |
| Abell 496 | 0135120201 | 0.0329 | 0.0458 | 17.8 | 17.6 | 14.1 | 1.397 (55) |
| PKS 0745-191 | 0105870101 | 0.1028 | 0.4240 | 18.9 | 18.9 | 9.8 | 0.944 (107) |
| Hydra A | 0109980301 | 0.0549 | 0.0494 | 18.6 | 19.8 | 15.8 | 1.266 (81) |
| Abell 1060 | 0206230101 | 0.0126 | 0.0490 | 40.0 | 41.5 | 33.2 | 2.588 (40) |
| Virgo (M87) | 0200920101 | 0.0044 | 0.0254 | 77.8 | 79.4 | 70.0 | 9.352 (51) |
| Centaurus | 0046340101 | 0.0114 | 0.0806 | 40.7 | 41.3 | 40.3 | 2.928 (41) |
| Abell 1644 | 0010420201 | 0.0473 | 0.0499 | 15.1 | 15.2 | 12.8 | 0.521 (29) |
| Abell 1650 | 0093200101 | 0.0838 | 0.0156 | 38.1 | 36.6 | 34.4 | 0.878 (83) |
| Abell 1651 | 0203020101 | 0.0849 | 0.0181 | 10.2 | 10.8 | 6.9 | 0.669 (64) |
| Abell 1689 | 0093030101 | 0.1830 | 0.0182 | 37.5 | 37.6 | 32.6 | 0.520 (96) |
| Abell 3558 | 0107260101 | 0.0480 | 0.0389 | 44.1 | 44.0 | 38.9 | 0.602 (34) |
| Abell 3562 | 0105261301 | 0.0490 | 0.0385 | 40.3 | 40.2 | 38.0 | 0.834 (48) |
| Abell 3571 | 0086950201 | 0.0391 | 0.0371 | 24.3 | 24.5 | 16.5 | 1.119 (52) |
| Abell 1795 | 0097820101 | 0.0625 | 0.0119 | 39.5 | 39.6 | 22.7 | 1.232 (89) |
| Abell 2029 | 0111270201 | 0.0773 | 0.0304 | 10.7 | 11.2 | 10.3 | 1.059 (93) |
| Abell 2052 | 0109920101 | 0.0355 | 0.0272 | 30.3 | 30.3 | 26.5 | 1.747 (74) |
| MKW3s | 0109930101 | 0.0450 | 0.0303 | 38.7 | 38.3 | 34.1 | 1.620 (86) |
| Abell 2065 | 0202080201 | 0.0726 | 0.0295 | 20.7 | 20.7 | 16.6 | 0.338 (28) |
| Abell 2063 | 0200120401 | 0.0349 | 0.0298 | 8.1 | 8.9 | 5.4 | 1.152 (48) |
| Abell 2199 | 0008030201 | 0.0302 | 0.0086 | 14.6 | 14.6 | 10.0 | 1.985 (72) |
| Abell 2204 | 0112230301 | 0.1523 | 0.0567 | 19.9 | 20.2 | 13.7 | 0.629 (100) |
| Cygnus A | 0302800101 | 0.0561 | 0.3490 | 22.2 | 22.2 | 20.2 | 1.041 (68) |
| Abell 2597 | 0147330101 | 0.0852 | 0.0249 | 52.2 | 53.3 | 48.5 | 0.792 (76) |
| Abell 4038 | 0204460101 | 0.0300 | 0.0155 | 29.4 | 29.2 | 27.6 | 1.859 (67) |
| Abell 4059e | 0109950101 | 0.0475 | 0.0110 | 12.7 | 13.7 | 7.0 | 1.378 (77) |
| Abell 4059 | 0109950201 | 0.0475 | 0.0110 | 23.3 | 23.2 | 19.7 | 1.378 (77) |
All objects are cool core
clusters with a mass deposition rate different from zero (Peres et al. 1998).
Notes: a redshifts taken from the NASA Extragalactic Database; b Galactic photoelectric absorption extracted from the HEASARCH Database (LAB survey Kalberla et al. 2005); c net exposure times for the three EPIC instruments after data cleaning in ks; d extraction radius is half the cooling radius from Peres et al. (1998); e the two observations of Abell 4059 were merged before the spectral analysis.
Notes: a redshifts taken from the NASA Extragalactic Database; b Galactic photoelectric absorption extracted from the HEASARCH Database (LAB survey Kalberla et al. 2005); c net exposure times for the three EPIC instruments after data cleaning in ks; d extraction radius is half the cooling radius from Peres et al. (1998); e the two observations of Abell 4059 were merged before the spectral analysis.
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