Table B.2.
Key properties of the semi-analytical models considered in this work, including star formation parameters.
| Halo catalog / merger tree | Feedback | Dust treatment | Star formation (ϵSF, nH) | |
|---|---|---|---|---|
| GAEA | Millennium + rescaling | SNe + AGN outflows | Includes self-consistent dust production and chemical enrichment | ϵSF ∼ 0.03–0.05, Schmidt-Kennicutt type law, nH ∼ 0.1 cm−3, T ∼ 104 K |
| L-GalP23 | Millennium | SNe + AGN (radio + quasar mode) | Dust treated via empirical/semi-analytic prescriptions | ϵSF ∼ 0.02–0.05, Kennicutt-Schmidt law, nH ∼ 0.1 cm−3, T ∼ 104 K |
Notes. For each semi-analytical model, the halo catalog, feedback implementation, dust treatment, and key star formation parameters are reported. Star formation efficiency (ϵSF) is per free-fall time and nH is the hydrogen number density threshold for SF.
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