Table C.1.
Properties of the best RPS models, and the model with the same spin and velocity but without the RPS for the galaxy VCC 2034.
| Galaxy | trps | λ | VC | log M⋆ | log Mgas | log SFR | Zgas |
|---|---|---|---|---|---|---|---|
| (Gyr) | (km s−1) | (M⊙) | (M⊙) | (M⊙ yr−1) | (Z⊙) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| Best-fit model | |||||||
| VCC 2034 | 13.55 ± 0.01 | 0.06 ± 0.01 | 44 ± 2 | 7.86 ± 0.04 | 7.09 ± 0.09 | −2.61 ± 0.01 | 1.87 ± 0.38 |
| Model without RPS | |||||||
| – | 0.06 ± 0.01 | 44 ± 2 | 7.88 ± 0.03 | 8.49 ± 0.09 | −1.36 ± 0.02 | 0.71 ± 0.14 | |
Notes. (1) Name of the galaxy; (2-4) Model parameters trps, λ and VC; (5-8) Stellar-mass, gas mass, SFR, and gas-phase metallicity predicted by the models. The uncertainties given in the best-fit models are from the confidence limits in trps, λ and VC parameters. For the non-RPS models, the uncertainties are from the error in λ and VC alone.
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