Table 1
Redshift zcluster and r500 of the clusters used in our study.
| Cluster | zcluster | r500 [kpc] | ![$\[N_{\mathrm{H}, \mathrm{TOT}}^{\text {neutral}(a)}\left[\mathrm{cm}^{-2}\right]\]$](/articles/aa/full_html/2025/02/aa51431-24/aa51431-24-eq18.png){kind=small} |
1 kpc [′] |
|---|---|---|---|---|
| A383 | 0.1883[1] | 944[1] | 3.88 × 1020 | 0.005 |
| A2029 | 0.0779[1] | 1362[1] | 3.70 × 1020 | 0.011 |
| A1795 | 0.0622[1] | 1235[1] | 1.24 × 1020 | 0.014 |
| Perseus | 0.01790[2] | 1245[2] | 20.7 × 1020 | 0.046 |
| A262 | 0.0162[1] | 650[1] | 7.15 × 1020 | 0.051 |
| NGC 4636 | 0.0037[3] | 350[3] | 2.07 × 1020 | 0.218 |
Notes. [1] Vikhlinin et al. (2006); [2] Hitomi Collaboration (2018b); [3] Pinto et al. (2015). (a) NH,TOT is the total hydrogen column density in the direction of the galaxy cluster, which was taken from Willingale et al. (2013). We used the online tool created by the SWIFT team, which is available here https://www.swift.ac.uk/analysis/nhtot/.
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