Table 2.
Summary of additional data and physical quantities used in this work.
| Quantity | Definition | Derived from dataset | Reference |
|---|---|---|---|
| ΣH2 | αCOICO(2 − 1)/R21(a) | ALMA | Leroy et al. (2021b) |
| E(B − V) | Equation (2) | MUSE | Groves et al. (2023) |
| Σ⋆ | Spectral fitting | MUSE | Emsellem et al. (2022) |
| sSFR | CHαIHα, corr/Σ⋆(b) | MUSE | Belfiore et al. (2023) |
| EW(Hα) | Moments of spectra (c) | MUSE | Groves et al. (2023) |
| 12 + log(O/H) | Scal. calibration (d) | MUSE | Groves et al. (2023) |
| log(U) | From  (e) |
MUSE | Groves et al. (2023) |
Notes.
Assuming a Milky Way conversion factor αCO = 4.35 M⊙ pc−2 (K km s−1)−1 (Bolatto et al. 2013) and a CO(2−1)-to-CO(1−0) ratio R21 = 0.65 (Den Brok et al. 2021).
log CHα/(M⊙ yr−1/(erg s−1)) = −41.26, from Calzetti et al. (2007).
Definition in Westfall et al. (2019).
Scal. calibration from Pilyugin & Grebel (2016).
Ionisation parameter calculated using the calibration from Diaz et al. (1991).
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