Table A.1.
Properties of the analyzed sample of galaxies. Stellar mass, SFR, and dust mass.
| Target name | log(M⋆/M⊙) | Reference | SFR [M⊙/yr] | Reference | log(Mdust/M⊙) | Reference |
|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| DLA0817g | ... | ... | 110 ± 10 | N17 | ... | ... |
| ALESS 073.1 | 10.7-11.1 | L21 | 1050 ± 150 FIR | G14 |
 |
G14 |
| HZ7 | 9.86 ± 0.21 | C15 |
 |
C15 | ... | ... |
| HZ9 | 9.86 ± 0.23 | C15 |
 |
P19 | ... | ... |
| HZ4 |
 |
F20 |
 |
F20 | ... | ... |
| J1211 | 10.47 | H20 | 86 | H20 |
 |
H20 |
| J0235 | 10.47 | H20 | 54 | H20 | ... | ... |
| CLM1 | 10.11 | W15 | 37 ± 4 SED | W15 | ... | ... |
| J0217 | 10.47 | H20 | 96 | H20 |
 |
H20 |
| VR7 | 10.23 | M17 |
 |
M19 | ... | ... |
| UVISTA-Z-349 |
 |
D22 |
 |
D22 |
 |
So22 |
| UVISTA-Z-004 |
 |
D22 |
 [C ii] |
F21 |
 |
So22 |
| UVISTA-Z-049 |
 |
D22 |
 |
D22 |
 |
So22 |
| UVISTA-Z-019 |
 |
Sc22 |
 |
W22 |
 |
W22 |
| COS-29 |
 |
S18 | 22.7±2.0UV | S18 | ..0. | ...00 |
| COS-30 |
 |
S18 | 19.2±1.6UV | S18 |
 |
W22 |
| UVISTA-Z-001 |
 |
Sc22 |
 |
W22 |
 |
W22 |
| UVISTA-Y-004 |
 |
D22 |
 |
D22 |
 |
So22 |
| UVISTA-Y-003 |
 |
D22 |
 |
D22 |
 |
So22 |
| UVISTA-Y-879 |
 |
D22 |
 |
D22 |
 |
So22 |
| SUPER8 |
 |
D22 |
 |
D22 |
 |
So22 |
| UVISTA-Y-001 |
 |
D22 |
 |
D22 |
 |
So22 |
References. G14 Gilli et al. (2014); C15 Capak et al. (2015); W15 Willott et al. (2015); M17 Matthee et al. (2017); N17 Neeleman et al. (2017); S18 Smit et al. (2018); M19 Matthee et al. (2019); P19 Pavesi et al. (2019); F20 Faisst et al. (2020); H20 Harikane et al. (2020); L21 Lelli et al. (2021); D22 Dayal et al. (2022); Sc22 Schouws et al. (2022); So22 Sommovigo et al. (2022); W22 Witstok et al. (2022).
Notes. (1): target name; (2) and (3): stellar masses computed from the UV luminosity and references; (4) and (5): SFR computed as SFR= SFRUV + SFRIR (if not indicated otherwise with a symbol) and references; (6) and (7): dust masses computed by SED fitting of the rest-frame FIR emission temperatures and references.
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