Table 2
Main cluster properties and simulation parameters of the baseline sample.
| Dynamical state | Sample | Index | M200 [h-1M⊙] | r200 [Mpc] | N gas | N dm | mgas [M⊙] | mdm [M⊙] | εgas [kpc] |
|
|
|
||||||||||
| perturbed (P) | S8 | 1 | 6 × 1014 | 1.96 | 220 175 | 220 144 | 3 × 109 | 1.5 × 1010 | 25.4 | −3.99 |
| S4 | 5 | 2.4 × 1014 | 1.45 | 221 007 | 220 976 | 2 × 109 | 1.1 × 1010 | 22.2 | −4.6 | |
| S4 | 16 | 2 × 1014 | 1.37 | 221 167 | 221 136 | 1.7 × 109 | 8.7 × 109 | 21 | −6.07 | |
| S2 | 105 | 6 × 1013 | 0.91 | 221 391 | 221 360 | 2.5 × 108 | 1.3 × 109 | 11.1 | −4.65 | |
|
|
||||||||||
| quiescent (Q) | S4 | 11 | 5.7 × 1014 | 1.94 | 220 759 | 220 728 | 1.5 × 109 | 7.6 × 109 | 20 | −7.46 |
| S4 | 19 | 7 × 1014 | 2.07 | 219 631 | 219 600 | 1.7 × 109 | 8.7 × 109 | 21 | −8.5 | |
| S2 | 13 | 2.4 × 1014 | 1.44 | 221 823 | 221 792 | 6.4 × 108 | 3.3 × 109 | 15.1 | −8.67 | |
| S2 | 110 | 9.4 × 1013 | 1.05 | 222 111 | 222 080 | 2.5 × 108 | 1.3 × 109 | 11.1 | −8.27 | |
Notes. From left to the right: the dynamical subset class, the cosmological sample membership, the corresponding sample index of the cluster, the present cluster mass M200 within r200 in units of h-1M⊙, the radius r200 is units of Mpc, the number of gas particles Ngas inside the Lc/2 sphere at z = zin, the same but for the dark matter particles, the mass of the gas particles mgas in M⊙, the same but for the dark matter particles, the gravitational softening parameter for the gas in kpc, and the root-mean-square plane average cluster power ratio 
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