Table 1.
Cluster properties and information of the XMM-Newton observations.
| Cluster | Obs. ID | MOS exposure | pn exposure | R500 | T | Flux (0.1 − 2.4 keV) | z |
|---|---|---|---|---|---|---|---|
| (ks) | (ks) | (Mpc) | (keV) | (erg s−1 cm−2) | |||
| Perseus | 0305780101 | 118 | 94 | 1.3 | 3.5 − 4.5 | 9.61 × 10−10 | 0.018 |
| 2A 0335+096 | 0147800201 | 79 | 76 | 0.9 | 2.4 − 3.5 | 9.16 × 10−11 | 0.036 |
| Sérsic 159−03 | 0147800101 | 86 | 77 | 0.8 | 2.5 − 2.7 | 2.49 × 10−11 | 0.056 |
Notes. ‘MOS Exposure’ and ‘pn Exposure’ are the effective exposure times of the MOS and pn cameras after the soft-proton cleaning. Estimates for R500 are taken from Giacintucci et al. (2019) for Perseus and 2A 0335+096, and from Sun et al. (2009) for Sérsic 159−03. Listed for each cluster are the temperature ranges covered by the various regions for which we extracted and fitted the spectra. These temperatures are in the ranges of interest. Regions with temperatures higher than 4.5 keV are not considered for Perseus, as explained in Sect. 3.2.1. The Perseus flux and redshift are from Ebeling et al. (2002); for 2A 0335+096 and Sérsic 159−03, we refer to de Plaa et al. (2007) and Sanders et al. (2011) for the flux and the redshift, respectively.
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