Table A.1.
Main properties of the sample of simulated massive discs studied in this work.
| Simulation | Galaxy ID | log10(M⋆/M⊙) | log10(Mhalo/M⊙) | vflat | Reff | ℛ⋆ | ℱ⋆ |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| EAGLE | 14582105 | 10.95 | 12.93 | 236.66 | 9.17 | 2.41 | 0.84 |
| EAGLE | 14202038 | 10.98 | 12.70 | 253.67 | 9.24 | 2.50 | 0.83 |
| EAGLE | 15518507 | 11.01 | 12.74 | 287.68 | 13.45 | 2.32 | 0.79 |
| ... | |||||||
| IllustrisTNG | 351452 | 11.11 | 12.48 | 266.92 | 9.20 | 1.75 | 0.82 |
| IllustrisTNG | 368436 | 11.33 | 12.64 | 290.15 | 16.58 | 1.79 | 0.84 |
| IllustrisTNG | 369366 | 10.89 | 12.25 | 225.96 | 13.18 | 1.82 | 0.89 |
| ... | |||||||
Notes. (1) Simulation suite: the runs analysed are Ref-L0100N1504 in EAGLE and TNG100-1 in IllustrisTNG; (2) galaxy ID from the catalogues of McAlpine et al. (2016) and Nelson et al. (2019); (3)-(4) stellar and halo masses; (5) velocity of the flat part of the rotation curve in km s−1, defined as specified in Sect. 2; (6) effective (half-mass) stellar radius in kpc; and (7)-(8) mean stellar v/σ and stellar disc fraction, defined as in Sect. 2.
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