Table 2.
Median properties for various sub-samples of galaxies from the MS sample.
| Sub-sample | Number | Proportion (%) | log10M⋆ | log10Mg | log10Mdyn | log10 SFRz | Reff,d |
|---|---|---|---|---|---|---|---|
| [M⊙] | [M⊙] | [M⊙] | [M⊙ yr−1] | [kpc] | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| Field | 256 | 57 |
 |
 |
 |
 |
 |
| Small | 56 | 13 |
 |
 |
 |
 |
 |
| Large | 135 | 30 |
 |
 |
 |
 |
 |
| Small-5 | 293 | 66 |
 |
 |
 |
 |
 |
| Large-5 | 154 | 34 |
 |
 |
 |
 |
 |
| Small-10 | 312 | 70 |
 |
 |
 |
 |
 |
| Small-15 | 345 | 77 |
 |
 |
 |
 |
 |
| Large-15 | 102 | 23 |
 |
 |
 |
 |
 |
| Small-20 | 370 | 83 |
 |
 |
 |
 |
 |
| Large-20 | 77 | 17 |
 |
 |
 |
 |
 |
Notes: (1) Sub-sample name (we do not show the Large-10 sub-sample since it is identical to the Large one), (2) number of galaxies in each sub-sample, (3) proportion of galaxies in each sub-sample, (4) SED-based stellar mass, (5) gas mass derived from the extinction corrected [O II] flux, (6) dynamical mass from the mass models, including the stellar disk, stellar bulge, and DM halo, (7) [O II]-based SFR normalised at redshift z0 ≈ 0.7, and (8) disk effective radius. Masses are computed within R22 = 2.2Rd, with Rd the disk scale length. Uncertainties correspond to the 16th and 84th percentiles.
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