Table 1.
Resolution parameters and number of total galaxies retained in the three different simulation suites at z = 0.
| AURIGA | HESTIA | NIHAO | |
|---|---|---|---|
| Resolution parameters | |||
| mdm [M⊙] | 3 × 105 | 1.2 × 106 | 1.7 × 106-3.4 × 103 |
| mgas [M⊙] | 5 × 104 | 1.8 × 105 | 3.2 × 105-6.2 × 102 |
| ϵz = 0 [pc] | 369 | 340 | 931.4–116.4 |
| Selection criteria | |||
| fMhires > 0.99 | 630 | 402 | 162 |
| Nstars > 100 | |||
Notes. The selection criteria used in each case can be found in the bottom left box. Host galaxies were selected based on a mass fraction of dark matter in high-resolution particles (fMhires) and a minimum number of star particles (Nstars) for each halo. For NIHAO simulation suites, we only show the maximum and minimum values of the resolution parameters, as well as the dark matter softening length.
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