Table 1.
Sample of galaxies resulting from the selection described in Section 3.1 for each simulation.
| Sim. | Mtot | ntotal | nbright | ndark | nstarless |
|---|---|---|---|---|---|
| (1012 M⊙) | |||||
| HESTIA 09_18 | 13.03 | 187 (27) | 84 (18) | 32 (0) | 17 |
| HESTIA 17_11 | 10.77 | 139 (14) | 56 (11) | 22 (0) | 11 |
| HESTIA 37_11 | 7.67 | 133 (25) | 53 (19) | 1 (1) | 0 |
| NIVARIA-LG | 5.51 | 81 (9) | 15 (4) | 59 (5) | 59 |
Notes. The first column lists the label assigned to each simulation. The second column provides the total mass contained within 2.5 Mpc of the corresponding MW analogue. The third column reports the total number of galaxies identified within 2.5 Mpc of the MW and with halo masses between 109 and 1010 M⊙ using the selection criteria. The fourth column shows the number of bright galaxies, while the fifth column lists the number of dark galaxies in each simulation. The final column displays the number of dark galaxies from the previous column that are completely starless. Values in brackets indicate galaxies that are satellites of others (i.e. systems that are not isolated).
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