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Table 2.
Physical properties of three examples of galaxies and their descendants.
| z | ID | Class | log(M⋆) | R⋆ | SFR |
|---|---|---|---|---|---|
| [M⊙] | [kpc] | [M⊙ yr−1] | |||
| (1) | (2) | (3) | (4) | (5) | (6) |
| 0.7 | 172231 | SF | 11.38 | 5.83 | 39.29 |
| 0.5 | 218606 | SF | 11.42 | 5.69 | 6.30 |
| 0.3 | 251598 | GV | 11.52 | 8.38 | 0.56 |
| 0.7 | 222130 | GV | 11.26 | 4.84 | 2.95 |
| 0.5 | 234935 | GV | 11.27 | 5.49 | 1.21 |
| 0.3 | 277675 | SF | 11.36 | 7.51 | 12.08 |
| 0.7 | 212087 | Q | 11.26 | 1.32 | 0.04 |
| 0.5 | 253460 | GV | 11.26 | 1.41 | 0.43 |
| 0.3 | 298351 | SF | 11.26 | 1.48 | 2.51 |
Notes. (1) Redshift. (2) Galaxy ID. (3) Class: SF = star forming, GV = green valley, Q = quiescent (see Croom et al. 2021). (4) Stellar mass within half-mass radius. (5) Half-mass stellar radius. (6) Global star formation rate.
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