Table 1.
Properties of the cluster sample.
| Cluster | Redshift | Distance | T3D | Rout | M⋆ | Mgas | Mbar |
|---|---|---|---|---|---|---|---|
| (Mpc) | (keV) | (Mpc) | (1014 M⊙) | (1014 M⊙) | (1014 M⊙) | ||
| Clusters without known merger signatures: | |||||||
| A1795 | 0.0622 | 279.7 ± 19.7 | 3.27 ± 0.19 | 2.4 | 0.08 | 1.1 | 1.18 |
| A2029 | 0.0766 | 350.7 ± 24.6 | 5.75 ± 0.27 | 2.7 | 0.22 | 2.2 | 2.42 |
| A2142 | 0.0900 | 397.7 ± 27.9 | 6.22 ± 0.27 | 2.8 | 0.24 | 2.6 | 2.84 |
| Clusters with known merger signatures: | |||||||
| A644 | 0.0704 | 315.3 ± 22.1 | 5.68 ±0.22 | 1.7 | 0.09 | 1.0 | 1.09 |
| A2319 | 0.0557 | 243.7 ± 17.1 | 7.21 ± 0.14 | 2.5 | 0.15 | 2.9 | 3.05 |
Notes. T3D is the deprojected ICM temperature averaged across all probed radii, Rout is the outermost radius at which gravitational accelerations are measured using the SZ effect (see Eckert et al. 2019), stellar mass (M⋆), gas mass (Mgas), and baryonic mass (Mbar) are measured within Rout; their uncertainties are of the order of 25%.
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