Table 1.
Summary of other wind studies.
| Paper | Ngal | zgal | SFRs | Galaxy type | log(M⋆/M⊙) | Method |
|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| Paper III | 27 | 0.5 < z < 1.5 | [O II] | SFGs | 8.5 − 11 | Background QSO |
| B12 | 5 | z ≈ 0.1 | SED | SFGs | 10 − 11 | Background QSO |
| S15 | 4 | 0.5 < z < 1.5 | [O II] | SFGs | 8.5 − 11 | Background QSO |
| H17 | 17 | z < 0.2 | SED | Starbursts | 10 − 11 | Background QSO |
| M19 | 16 | z < 0.4 | SED | SFGs | 9 − 11 | Background QSO |
| H15 | 32 | z < 0.2 | SED | Starbursts | 7 − 11 | Down-the-barrel |
| P23 | 14 | z ≈ 0.5 | SED | Starbursts | 10.5 − 11.2 | Down-the-barrel |
Notes. (1) Study name, Paper III for Schroetter et al. (2019), B12 for Bouché et al. (2012), S15 for the SIMPLE wind cases in Schroetter et al. (2015), H15 and H17 respectively for Heckman et al. (2015 and 2017), M19 for Martin et al. (2019), and P23 for Perrotta et al. (2023); (2) Sample size in galaxy number. (3) Redshift range; (4) Method used to estimate galaxy SFR; (5) Type of galaxy; (6) Galaxy stellar mass range; (7) Method used to constrain outflow properties.
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