Table 1.
Properties of the DIANOGA PCs.
| ID | M200c, z = 0 | M200c, MP | Radius | Nc |
|---|---|---|---|---|
| [1014 M⊙] | [1013 M⊙] | [Mpc] | ||
| 1 | 5.2 | 3.4 | 3.9 | 2 |
| 2 | 7.6 | 4.8 | 4.4 | 3 |
| 3 | 6.0 | 1.8 | 4.0 | 1 |
| 4 | 1.8 | 4.0 | 2.1 | 1 |
| 5 | 16 | 8.9 | 6.2 | 2 |
| 6 | 16 | 12 | 6.0 | 4 |
| 7 | 1.5 | 2.8 | 2.1 | 1 |
| 8 | 15 | 7.0 | 5.3 | 6 |
| 9 | 18 | 3.2 | 7.9 | 8 |
| 10 | 18 | 11 | 7.1 | 4 |
| 11 | 32 | 9.1 | 6.7 | 7 |
| 12 | 18 | 8.3 | 6.5 | 5 |
| 13 | 18 | 11 | 6.2 | 2 |
| 14 | 11 | 3.4 | 5.5 | 3 |
Notes. Reported above are the ID, the mass of the z = 0 cluster, the mass of the main progenitor halo at z = 2.2, the radius of the PC region and the number of PC cores (halos with M200c > 1.5 × 1013 M⊙ within the PC region) for each DIANOGA PC. The z = 0 masses of the clusters with ID 10 and 11, that were not simulated to z = 0, come from the parent DM simulation.
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