Table 1.
Galaxy samples.
| Name | ng | fg | nMM |
|---|---|---|---|
| PS (parent sample) | 198 | 1.0 | 94 |
| BL (B/D ≤ 0.08) | 31 | 0.15 | 14 |
| BD (B/D > 1) | 32 | 0.16 | 16 |
Notes. Parent sample (PS, Pillepich et al. 2024), Bulgeless (BL) and bulge-dominated (BD). BL and BD samples are distinguished based on the stellar mass ratio of the bulge to the thin disc (B/D). Columns from left to right list: name of the sample, number of galaxies in each subsample, fraction relative to PS, number of galaxies which experienced at least one major merger since z = 2.
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