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Table 1
XMM-Newton-EPIC observations used in our analysis, with effective exposure time corresponding to each instrument.
| Cluster name | XMM-Newton | Center coordinates | MOS1 effective | MOS2 effective | PN effective |
| obs. IDs | exposure time (ks) | exposure time (ks) | exposure time (ks) | ||
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| A2933 | 0305060101 | 01h40m41.2s −54°33′26.0′′ | 21.5 (69.3%) | 27.7 (89.0%) | 16.3 (68.5 %) |
| A2440 | 0401920101 | 22h23m52.6s −01°36′57.0′′ | 25.3 (55.4%) | 24.9 (54.3%) | 17.8 (50.3 %) |
| A2384 | 0101902701 | 21h52m14.2s −19°42′19.8′′ | 17.2 (65.4%) | 16.8 (63.6%) | 10.2 (51.6 %) |
Notes. In brackets: fraction of the useful exposure time after solar-flare “cleaning”.
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