Table 1.
Properties of SERRA galaxies analyzed in this work.
| Name | z | M⋆ | Mg | SFR | L[CII] |
|---|---|---|---|---|---|
| [1010 M⊙] | [109 M⊙] | [M⊙ yr−1] | [108 L⊙] | ||
| Opuntia | 6.1 | 1.2 | 4.5 | 19 | 3.1 |
| Lantana | 6.4 | 1.7 | 7 | 44 | 6.6 |
| Petunia | 7.0 | 1.8 | 2.8 | 116 | 5.1 |
| Freesia | 6.5 | 1.1 | 3.8 | 44 | 5.0 |
| Adenia | 6.5 | 1.9 | 5.4 | 51 | 3.4 |
| Fuchsia | 7.2 | 0.3 | 1.7 | 24 | 1.0 |
Notes. M⋆ is the stellar mass, Mg is the gas mass, SFR is the star formation rate SFR and L[CII] is the [C II] line luminosity (see Pallottini et al. 2022; Kohandel et al., in prep.). Opuntia, Lantana and Petunia are the three disk galaxies, Freesia is the disturbed disk, and Adenia and Fuchsia are the two mergers.
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