Table 3.
Results of the sample of DGS galaxies and LBGs that have been individually fitted through the models provided in Table 2.
| Name |  |
Msil × 10−4 | Mcar × 10−4 | Mir × 10−4 | fcond | Mgas | α | Mswept × 103 | fdust, out | fgas, out | fdust, out/(out + SN) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| DGS galaxies | |||||||||||
| Haro 3 | 4.76 | 21.4 ± 3.6 | 4.8 ± 1.3 | 4.04 ± 0.72 | 0.44 ± 0.26 | 36 ± 14 | 1.24 ± 0.22 | 4.2 ± 2.9 | 0.44 ± 0.26 | 0.58 ± 0.29 | 0.66 ± 0.25 |
| He2-10 | 12.1 | 18.3 ± 0.8 | 5.84 ± 0.47 | 3.64 ± 0.19 | 0.25 ± 0.00 | 20.0 ± 0.0 | 1.42 ± 0.07 | 6.80 ± 0.23 | 0.21 ± 0.02 | 0.32 ± 0.03 | 0.21 ± 0.03 |
| HS 0052+2536 | 5.38 | 14.9 ± 8.2 | 3.39 ± 1.95 | 2.62 ± 1.50 | 0.28 ± 0.08 | 36 ± 21 | 1.29 ± 0.21 | 4.4 ± 2.9 | 0.25 ± 0.20 | 0.38 ± 0.26 | 0.63 ± 0.26 |
| HS 0822+3542 | 55.1 | 12.2 ± 1.5 | 2.41 ± 0.29 | 2.03 ± 0.25 | 0.25 ± 0.00 | 100.0 ± 0.7 | 1.00 ± 0.00 | 6.2 ± 1.7 | 0.24 ± 0.06 | 0.41 ± 0.08 | 0.85 ± 0.06 |
| … | |||||||||||
| LBGs | |||||||||||
| ID27 | 1.61 | 10 ± 11 | 1.3 ± 1.3 | 1.6 ± 1.8 | 0.61 ± 0.32 | 55 ± 29 | 1.28 ± 0.21 | 3.9 ± 2.9 | 0.06 ± 0.07 | 0.12 ± 0.13 | 0.79 ± 0.21 |
| ID31 | 1.14 | 16 ± 14 | 2.3 ± 1.8 | 2.6 ± 2.4 | 0.60 ± 0.31 | 55 ± 29 | 1.28 ± 0.21 | 3.9 ± 2.9 | 0.10 ± 0.12 | 0.19 ± 0.18 | 0.76 ± 0.22 |
| lbg10 | 1.96 | 29 ± 24 | 4.1 ± 2.7 | 4.8 ± 4.0 | 0.61 ± 0.32 | 55 ± 29 | 1.28 ± 0.21 | 3.9 ± 2.9 | 0.20 ± 0.19 | 0.32 ± 0.25 | 0.72 ± 0.23 |
| HZ4 | 2.20 | 36 ± 15 | 6.9 ± 2.9 | 6.2 ± 2.6 | 0.52 ± 0.27 | 56 ± 28 | 1.27 ± 0.21 | 3.9 ± 2.9 | 0.31 ± 0.22 | 0.46 ± 0.27 | 0.67 ± 0.25 |
| … | |||||||||||
Notes. For each of the galaxies analysed, we provide the averaged residual, the predicted mass of the different dust components (silicates, carbon and iron) normalised for the final stellar mass, the dust condensation fraction for SNe II, the initial mass of baryons normalised for the final stellar mass, the slope of the top-heavy IMF, the Mswept in M⊙, the fraction of the dust in the circumgalactic medium over the total (fdust, out), the fraction of gas in the circumgalactic medium over the total (fgas, out), and the ratio between the dust removed by the galactic outflow and the total removed and destroyed (fdust, out/(out + SN)). The complete table is provided at the CDS.
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