Table 2.
XMM-Newton observations for the galaxy clusters of this work.
| Cluster name | ObsIDs | texp [ks] | NH [1020 cm−2] |
|---|---|---|---|
| PSZ2 G259.98-63.43 | 0042340301 | 37.3 (95.4%), 38.4 (94.6%), 24.5 (80.1%) | 1.99 |
| 0827350201 | |||
| PSZ2 G262.73-40.92 | 0656201601 | 54.1 (83%), 56.1 (85.9%), 38.4 (75%) | 1.08 |
| 0827360501 | |||
| PSZ2 G263.68-22.55 | 0201901201 | 26.8 (49.3%), 29.4 (53.9%), 14 (54.5%) | 6.88 |
| 0201903401 | |||
| 0404910401 | |||
| PSZ2 G271.18-30.95 | 0656201301 | 28.5 (44.9%), 32.5 (51.1%), 23.6 (52.6%) | 4.28 |
| 0827050701 | |||
| PSZ2 G277.76-51.74 | 0656200301 | 56 (72.6%), 31.3 (40.5%), 37.5 (65.9%) | 1.85 |
| 0674380301 | |||
| PSZ2 G339.63-69.34 | 0693661801 | 210.8 (87.4%), 214.4 (88.8%), 131 (62.4%) | 1.39 |
| 0722700101 | |||
| 0722700201 | |||
Notes. The clean exposure times texp (after the light-curve filtering; see Sect. 3.2) and the relative percentage (relative to the total available) correspond to the sum of the exposures of the listed observations for the three EPIC cameras (MOS1, MOS2, and PN). The NH column contains the total (HI plus molecular) hydrogen column density estimated in Bourdin et al. (in prep.).
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