Table 1.
List of some general properties of the galaxy clusters analyzed in this study.
| Cluster ID | M200 | M200gas | R200 | R500 | R2500 | Active/ |
|---|---|---|---|---|---|---|
| [1015 h−1 M⊙] | [h−1 Mpc] | Relaxed | ||||
| g1212639 | 1.9 | 0.28 | 3.2 | 2.2 | 0.5 | 61%/ 39% |
| g1483463 | 1.6 | 0.24 | 3.1 | 2.2 | 0.4 | 100%/ 0% |
| g1657050 | 1.9 | 0.29 | 3.2 | 2.1 | 0.5 | 47%/ 53% |
| g1680241 | 1.7 | 0.26 | 3.1 | 2.0 | 0.4 | 89%/ 11% |
| g1987669 | 1.9 | 0.29 | 3.2 | 2.3 | 0.5 | 96%/ 4% |
| g5503149 | 1.6 | 0.25 | 3.1 | 2.1 | 0.5 | 88%/ 12% |
| g6348555 | 1.7 | 0.28 | 3.1 | 2.1 | 0.5 | 0%/100% |
Notes. The bold part of the identification number is used as an abbreviation in the text. The last column gives the fraction of the evolution time since z = 0.43 that the cluster is relaxed or active. The dynamical state was determined by the method described in Sect. 3.1. All properties agree between MFM and SPH in the given accuracy and differences are ≲1%.
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