Table 1.
Sample of high-redshift galaxies with observed ionised gas outflows.
| ID | z | log(M*/M⊙) | log(SFR/M⊙ yr−1) | log(Mout/M⊙) | rout [kpc] | vout [km s−1] | log (Ṁout/M⊙ yr−1) | log(η) |
|---|---|---|---|---|---|---|---|---|
| [O III] | ||||||||
| 5457 | 4.861 | 7.69 ± 0.05 | 0.09 ± 0.19 | 6.46 ± 0.02 | 0.21 | 500 ± 55 | 0.84 ± 0.30 | 0.8 ± 0.3 |
| 9422 | 5.935 | 7.60 ± 0.02 | 0.53 ± 0.00 | 7.07 ± 0.01 | 0.30 | 234 ± 77 | 0.91 ± 0.30 | 0.4 ± 0.3 |
| 18090 | 4.773 | 7.85 ± 0.05 | 0.61 ± 0.02 | 6.84 ± 0.02 | 0.64 | 701 ± 53 | 0.88 ± 0.30 | 0.3 ± 0.3 |
| 18846 | 6.334 | 8.09 ± 0.02 | 0.39 ± 0.01 | 6.56 ± 0.01 | 0.52 | 401 ± 50 | 0.43 ± 0.30 | 0.0 ± 0.3 |
| 10013609 | 6.928 | 7.78 ± 0.07 | 0.41 ± 0.02 | 7.12 ± 0.01 | 0.33 | 259 ± 46 | 0.97 ± 0.30 | 0.6 ± 0.3 |
| 10013704 | 5.919 | 8.63 ± 0.02 | 1.14 ± 0.02 | 8.26 ± 0.01 | 0.31 | 289 ± 53 | 2.22 ± 0.30 | 1.1 ± 0.3 |
| Hα | ||||||||
| 3184 | 3.467 | 8.54 ± 0.05 | 0.65 ± 0.06 | 6.74 ± 0.01 | 0.71 | 267 ± 46 | 0.29 ± 0.30 | −0.4 ± 0.3 |
| 4270 | 4.022 | 8.11 ± 0.02 | 0.74 ± 0.01 | 7.17 ± 0.02 | 0.44 | 444 ± 74 | 1.17 ± 0.30 | 0.4 ± 0.3 |
| 6246 | 5.560 | 7.73 ± 0.12 | 0.14 ± 0.05 | 6.00 ± 0.02 | 0.29 | 497 ± 44 | 0.24 ± 0.30 | 0.1 ± 0.3 |
| 7762 | 4.148 | 8.28 ± 0.01 | 0.34 ± 0.02 | 6.54 ± 0.01 | 0.61 | 229 ± 42 | 0.07 ± 0.30 | −0.3 ± 0.3 |
| 7892 | 4.228 | 7.81 ± 0.04 | 0.09 ± 0.01 | 6.03 ± 0.01 | 0.10 | 275 ± 56 | 0.45 ± 0.30 | 0.4 ± 0.3 |
| 17260 | 4.885 | 7.93 ± 0.31 | −0.67 ± 0.04 | 5.85 ± 0.02 | 0.17 | 648 ± 50 | 0.43 ± 0.30 | 1.1 ± 0.3 |
| 18090 | 4.773 | 7.85 ± 0.05 | 0.61 ± 0.02 | 6.67 ± 0.01 | 0.64 | 261 ± 59 | 0.25 ± 0.30 | −0.4 ± 0.3 |
| 10016186 | 3.927 | 8.24 ± 0.01 | 0.01 ± 0.02 | 6.51 ± 0.02 | 4.06 | 911 ± 67 | −0.13 ± 0.30 | −0.1 ± 0.3 |
Notes. This sample of observed galaxies is used for comparison with the theoretical predictions presented in this work. The ID corresponds to the NIRSpec ID of the target, the outflow radius rout is assumed to coincide with the galaxy radius, and the mass-loading factor is defined as η ≡ Ṁout/SFR. The table is reproduced from Carniani et al. (2024).
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