Table B.1.
Key properties of the hydrodynamical simulations considered in this work, including star formation (SF) parameters.
| Box-size [Mpc/h] | Baryonic mass resolution [M⊙] | Spatial resolution [kpc] | Feedback | Dust treatment | Star formation (ϵSF, nH) | |
|---|---|---|---|---|---|---|
| EAGLE | 100 | ∼1.8 × 106 | ∼0.7 | SNe + AGN heating | Not self-consistent; post-processed dust models available | ϵSF ∼ 0.02, nH = 0.1 (Z/0.002)−0.64 cm−3 |
| IllustrisTNG | 110 | ∼1.4 × 106 | ∼1.0 | SNe (winds) + AGN (kinetic + thermal) | Not self-consistent; dust added in post-processing | ϵSF ∼ 0.02, nH ∼ 0.1–0.3 cm−3 (metallicity-dependent) |
| SIMBA | 150 | ∼1.8 × 107 | ∼1.5 | SNe + AGN (radiative + jets) | Includes self-consistent dust production and destruction | ϵSF ∼ 0.02, SF model based on molecular hydrogen fraction |
Notes. For each hydrodynamical simulation, the simulated volume, resolution, 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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.