Table 2.
Cluster haloes studied in this work.
| Name | 1 × R15 | 1 × RF18 | 10 × B20 | 1 × B20 | ||||
|---|---|---|---|---|---|---|---|---|
| Mvir | Ns | Mvir | Ns | Mvir | Ns | Mvir | Ns | |
| D1 | 11.4 | 62 | 11.4 | 38 | 11.1 | 87 | ||
| D3 | 4.9 | 25 | 4.8 | 13 | 4.8 | 28 | 4.8 | 21 |
| D6 | 6.3 | 28 | 6.3 | 25 | 6.4 | 42 | 6.4 | 34 |
| D10 | 10.4 | 70 | 10.4 | 48 | 10.1 | 83 | ||
| D18 | 8.0 | 32 | 8.1 | 23 | 7.7 | 49 | 7.6 | 31 |
| D25 | 3.1 | 13 | 3.0 | 12 | 3.0 | 22 | 2.3 | 13 |
Notes. First column reports the names of the 6 out of the 29 Dianoga regions used in this work. The panels in other columns are the halo virial masses (Mvir) and the number Ns of SHs with mass MSH > 2 × 1010 h−1 M⊙ within a distance of r < 0.15Rvir from the halo centre. These quantities are reported for all suites (1 × R15, 1 × RF18, 10×, and 1 × B20). Virial masses are in units of 1014 h−1 M⊙. Haloes are extracted at redshift z = 0.4.
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