Table 1.
Descendant galaxy samples defined according to their final morphology (z = 0).
| Name | (D/T)thin, z1 | (D/T)thin, z0 | ngal | fgal | nbar, z1 | nbar, z0 | nbar, form, z < 1 | nbar, lost, z < 1 | nunbar, z1 | nunbar, z0 |
|---|---|---|---|---|---|---|---|---|---|---|
| Parent sample | 0.67 | 0.18 | 204 | 1 | 93 | 115 | 59 | 6 | 111 | 36 |
| Disc descendants | ≥0.5 | ≥0.5 | 104 | 0.51 | 36 | 74 | 43 | 5 | 68 | 30 |
| Lenticular descendants | ≥0.5 | ≥0.3, < 0.5 | 47 | 0.23 | 26 | 41 | 16 | 1 | 22 | 6 |
| Spheroidal descendant | ≥0.5 | < 0.3 | 53 | 0.26 | 31 | – | – | – | 21 | – |
Notes. From left to right: sample name, thin-disc mass fraction (D/T)thin at z = 1 ((D/T)thin, z1), (D/T)thin at z = 0 ((D/T)thin, z0), number of galaxies, the fraction with respect to the parent disc sample at z = 1 (fgal), number of bars at z = 1 (nbar, z1), number of bars at z = 0 (nbar, z0), number of bars formed after z = 1 nbar, form, z < 1, number of dissolved bars (nbar, lost, z < 1), number of unbarred galaxies (nunbar, z = 1), and number of unbarred galaxies at z = 0 (nunbar, z = 0).
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