Table A.2
Best-fit temperatures and 68% confidence levels for the 4 different detectors (plus EPIC combined) in the (0.7−7) keV band.
| Cluster name | k T ACIS | k T MOS1 | k T MOS2 | k T PN | k T EPIC, Combined | SC/BKG |
| [keV] | [keV] | [keV] | [keV] | [keV] | ||
|
|
||||||
| 2A0335 |
|
|
|
|
|
25.69 |
| A0085 |
|
|
|
|
|
71.51 |
| A0119 |
|
|
|
|
|
21.97 |
| A0133 |
|
|
|
|
|
22.71 |
| A0262 |
|
|
|
|
|
24.69 |
| A0399 |
|
|
|
|
|
48.96 |
| A0400 |
|
|
|
|
|
22.36 |
| A0401 |
|
|
|
|
|
77.50 |
| A0478 |
|
|
|
|
|
49.05 |
| A0496 |
|
|
|
|
|
41.73 |
| A0576 |
|
|
|
|
|
29.60 |
| A0754 |
|
|
|
|
|
75.28 |
| A1060 |
|
|
|
|
|
92.29 |
| A1367 |
|
|
|
|
|
13.92 |
| A1644 |
|
|
|
|
|
22.80 |
| A1650 |
|
|
|
|
|
55.96 |
| A1651 |
|
|
|
|
|
97.23 |
| A1656 |
|
|
|
|
|
88.21 |
| A1736 |
|
|
|
|
|
28.06 |
| A1795 |
|
|
|
|
|
55.67 |
| A2029 |
|
|
|
|
|
71.64 |
| A2052 |
|
|
|
|
|
31.28 |
| A2063 |
|
|
|
|
|
44.95 |
| A2065 |
|
|
|
|
|
36.67 |
| A2142 | – | – | – | – | – | – |
| A2147 |
|
|
|
|
|
39.33 |
| A2163 |
|
|
|
|
|
65.74 |
| A2199 |
|
|
|
|
|
103.19 |
| A2204 |
|
|
|
|
|
28.37 |
| A2255 |
|
|
|
|
|
25.73 |
| A2256 | – | – | – | – | – | – |
| A2589 |
|
|
|
|
|
25.80 |
| A2597 |
|
|
|
|
|
14.65 |
| A2634 |
|
|
|
|
|
10.60 |
| A2657 |
|
|
|
|
|
45.92 |
| A3112 |
|
|
|
|
|
33.10 |
| A3158 |
|
|
|
|
|
83.88 |
| A3266 |
|
|
|
|
|
93.71 |
| A3376 |
|
|
|
|
|
17.92 |
| A3391 |
|
|
|
|
|
34.57 |
| A3395 |
|
|
|
|
|
15.67 |
| A3526 | – | – | – | – | – | – |
| A3558 |
|
|
|
|
|
55.17 |
| A3562 |
|
|
|
|
|
50.44 |
| A3571 |
|
|
|
|
|
135.09 |
| A3581 |
|
|
|
|
|
17.71 |
| A3667 |
|
|
|
|
|
58.63 |
| A4038 |
|
|
|
|
|
109.43 |
| A4059 |
|
|
|
|
|
40.47 |
| EXO0422 |
|
|
|
|
|
48.04 |
| HydraA | – | – | – | – | – | – |
| IIIZw54 |
|
|
|
|
|
34.60 |
| MKW3S |
|
|
|
|
|
57.74 |
| MKW4 |
|
|
|
|
|
17.30 |
| MKW8 |
|
|
|
|
|
18.74 |
| NGC 1399 | – | – | – | – | – | – |
| NGC 1550 |
|
|
|
|
|
28.38 |
| NGC 4636 | – | – | – | – | – | – |
| NGC 5044 | – | – | – | – | – | – |
| NGC 507 |
|
|
|
|
|
21.37 |
| RXC J1504 |
|
|
|
|
|
8.87 |
| S1101 |
|
|
|
|
|
20.09 |
| ZwCl1215 |
|
|
|
|
|
59.56 |
Notes. The annulus region was used for cool-core clusters. For details on the excluded spectra, see Sect. 2. The last column gives the ratio of source and background count rates in the (0.7−2.0) keV band.
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