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Table 2.
Parameters used for SED fitting with BAGPIPES.
| Parameter | Quantity | Prior |
|---|---|---|
| Redshift, z | fixed | Spectroscopic redshift |
| Metallicity, Z | varied | [0.05; 1.3] Z⊙ |
| Ionization parameter, log𝒰 | varied | [ − 3; −1] |
| Max age of birth clouds, tbc | fixed | 10 Myr |
| Dust | ||
| Extinction curve model | fixed | Calzetti et al. (2000) |
| Dust emission model | fixed | Draine & Li (2007) |
| V-band extinction AV | varied | [0; 3] |
| Delayed exponential SFH | ||
| Initial mass function | fixed | Kroupa (2001) |
| Stellar population model | fixed | Bruzual & Charlot (2003) |
| Starting SFR age | varied | [0.002; 9.5] Gyr |
| Timescale of decrease | varied | [0.002; 9.5] Gyr |
| Mass formed | varied | [104; 1010] M⊙ |
Notes. All the priors are uniform. When two delayed exponentials are used, the parameters described in the SFH section are valid for both.
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