Table 3.
Main properties of the simulated systems studied in this work.
ID | M200 | M⋆ | MHI | SFR |
---|---|---|---|---|
[1012 M⊙] | [1010 M⊙] | [1010 M⊙] | [M⊙ yr−1] | |
(1) | (2) | (3) | (4) | (5) |
TNG50 | ||||
459557 | 0.81 | 4.50 | 1.67 | 1.34 |
476266 | 1.45 | 5.02 | 2.27 | 6.93 |
477328 | 1.95 | 6.22 | 3.32 | 8.91 |
517271 | 1.41 | 6.44 | 1.21 | 2.06 |
520885 | 1.17 | 5.47 | 3.17 | 2.90 |
522530 | 1.29 | 6.89 | 1.63 | 1.55 |
526478 | 1.12 | 4.84 | 2.60 | 7.40 |
531320 | 1.15 | 3.98 | 2.31 | 2.29 |
537488 | 0.95 | 4.38 | 0.89 | 3.15 |
537941 | 0.95 | 5.24 | 1.85 | 4.31 |
543376 | 0.93 | 6.14 | 1.11 | 4.14 |
543729 | 0.95 | 4.93 | 1.70 | 6.05 |
550934 | 0.89 | 3.56 | 1.77 | 4.72 |
554798 | 0.87 | 5.33 | 0.74 | 1.23 |
555013 | 0.89 | 3.66 | 1.85 | 1.46 |
555287 | 0.78 | 3.85 | 1.44 | 4.56 |
555601 | 0.78 | 4.60 | 1.75 | 4.49 |
559036 | 0.72 | 3.40 | 2.10 | 3.23 |
565251 | 0.71 | 3.55 | 0.62 | 3.60 |
566365 | 0.68 | 3.25 | 0.44 | 3.36 |
FIRE-2 | ||||
m12b | 1.43 | 9.93 | 1.13 | 9.04 |
m12f | 1.71 | 9.59 | 2.70 | 10.94 |
m12i | 1.18 | 7.26 | 1.27 | 6.97 |
m12r | 1.10 | 2.06 | 1.13 | 2.39 |
m12w | 1.08 | 6.52 | 0.25 | 10.79 |
Notes. (1) Simulated galaxy ID. For TNG50 systems this refers to the subhalo index in the group catalogues, as determined by the SUBFIND algorithm (Dolag et al. 2009). For FIRE-2 systems it refers to the run name in Wetzel et al. (2023). (2) Halo mass, computed within the radius where the mean halo density becomes equal to 200 times the critical density of the Universe. (3)–(5) Stellar mass, H I mass, and instantaneous SFR computed within 100 kpc from the centre of each galaxy.
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