Table 2.
cosmosTNG small-scale variation runs.
| Suffix | Ngal | SFRDz = 2 | MZFIRE, max |
|---|---|---|---|
| (M⋆ > 108 M⊙) | [10−2 M⊙/yr/cMpc3] | [1013 M⊙] | |
| A | 432 | 8.13 | 2.50 |
| B | 483 | 9.13 | 2.87 |
| C | 491 | 8.41 | 1.56 |
| D | 453 | 8.67 | 2.30 |
| E | 473 | 8.88 | 2.48 |
| F | 451 | 8.45 | 1.76 |
| G | 472 | 8.95 | 2.85 |
| H | 482 | 8.49 | 2.87 |
| 467 ± 19 | 8.64 ± 0.31 | 2.40 ± 0.47 | |
Notes. The shown properties from each volume highlight the diversity that results from varying the small-scale (unconstrained) power. These are the number of galaxies with stellar mass above 108 M⊙ (Ngal), the average instantaneous star formation rate density (SFRD), and the mass of the most massive halo in the zoomed-in region (MZFIRE, max; upper right panel of Fig. 5). All simulations are run to z = 2, where these properties are measured. The last line shows the mean and standard deviation of the variation runs.
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