Table 2.
Resolution of our simulations.
| ID merger tree | N(< 5rinf) – LR | mBH/m* – LR | N(< 5rinf) – HR | mBH/m* – HR |
|---|---|---|---|---|
| 17187 | 261 467 | 21 392.6 | 523 021 | 42 785.2 |
| 125027 | 279 200 | 24 236.9 | 558 279 | 48 473.8 |
| 125028 | 270 623 | 22 935.4 | 540 984 | 45 870.9 |
| 168390 | 205 663 | 14 892.5 | 411 478 | 29 785.1 |
| 197109 | 117 610 | 6240.8 | 234 907 | 12 481.7 |
Notes. For each merger tree, we report: (i) the number of stellar and DM particles within five influence radii (N(< 5rinf)), computed for the primary galaxy of the first merger of each merger tree; and (ii) the ratio between the primary BH mass and the mass of star particles in the innermost region (mBH/m*).
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