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Table 2.
Properties of the clusters sampled in our six zoom-in simulations of galaxies.
| Simulation | Total mass in clusters | Massive clusters | α |
|---|---|---|---|
| [M⊙] | |||
| m11i | 8.65 × 107 | 5 | −2.99 |
| m11q | 7.96 × 107 | 1 | −3.48 |
| m11e | 1.43 × 108 | 20 | −2.93 |
| m11h | 3.09 × 108 | 97 | −2.70 |
| m11d | 5.72 × 108 | 482 | −2.39 |
| m12i | 1.37 × 1010 | 8575 | −2.55 |
Notes. The selection criterion of massive clusters is Mcl ≥ 6 × 104 M⊙. It is only applied at the epoch the cluster is formed. The α parameter corresponds to the best fit power-law index described in Eq. (6).
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