Table 1.
Physical properties of the final sample.
| Cls | N | δ | log(sSFR) | log(Mstar) | Re | n | D4000 | FUV − NUV |
|---|---|---|---|---|---|---|---|---|
| C1 | 3061 |  |
 |
 |
 |
 |
 |
 |
| C2 | 1637 |  |
 |
 |
 |
 |
 |
 |
| C3 | 2478 |  |
 |
 |
 |
 |
 |
 |
| C1–3 | 7176 |  |
 |
 |
 |
 |
 |
 |
| C4 | 2801 |  |
 |
 |
 |
 |
 |
 |
| C5 | 2270 |  |
 |
 |
 |
 |
 |
 |
| C6 | 688 |  |
 |
 |
 |
 |
 |
 |
| C4–6 | 5759 |  |
 |
 |
 |
 |
 |
 |
| C7 | 3281 |  |
 |
 |
 |
 |
 |
 |
| C8 | 1203 |  |
 |
 |
 |
 |
 |
 |
| C9 | 3468 |  |
 |
 |
 |
 |
 |
 |
| C10 | 9207 |  |
 |
 |
 |
 |
 |
 |
| C11 | 1537 |  |
 |
 |
 |
 |
 |
 |
| C7–11 | 18696 |  |
 |
 |
 |
 |
 |
 |
Notes. The number of galaxies (N), median values of δ, specific star formation rate, log(sSFR) [yr−1], stellar mass, log(Mstar/M⊙), effective radius, Re [kpc], Sérsic index, n, D4000 and rest-frame FUV − NUV colour for each sub-class, Cls, are provided. Errors correspond to the differences between median and the first and the third quartile, respectively.
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