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Table E.1.

Non-exhaustive summary of the hydrodynamical simulations used in this work.

Simulation Box size Resolution Mass resolution Cosmology Dataset used in this work Halo mass definition Key comments
HORIZON-AGNa (Dubois et al. 2014) 100 h−1cMpc 10243 DM: 8 × 107 M Stars: 2 × 106 M WMAP-7 Galaxy and halo catalogs from a light-cone of 1 deg2 area from redshift z = 0 to z = 6 (Laigle et al. 2019; Gouin et al. 2019) Sum of all DM particles in the main subhalo AGN feedback; Overestimates SMF for log(M/M)≥9.5 (Kaviraj et al. 2017) and underestimates at z > 4 due to spatial resolution limitations (see Hatfield et al. 2019; Shuntov et al. 2022); Chabrier (2003) IMF.

TNG100b (Pillepich et al. 2018; Nelson et al. 2018; Marinacci et al. 2018; Naiman et al. 2018; Springel et al. 2018) 75 h−1cMpc 18203 DM: 7.5 × 106 M Stars: 1.6 × 106 M Planck+16 Public galaxy and halo catalogs from snapshots Sum of all DM particles in the main subhalo Calibrated on low-z data; Chabrier (2003) IMF.

THESANc (Kannan et al. 2022) 64.7 h−1cMpc 21003 DM: 3.12 × 106 M Stars: 5.8 × 105 M Planck+16 Galaxy catalogs from the public database Virial mass Epoch of reionization; IllustrisTNG model + radiative transfer; Chabrier (2003) IMF.

FirstLightd (Ceverino et al. 2017) 10–80 h−1Mpc 81923 DM: 104 M Stars: 106 M Planck+16 Public database that contains information on 377 galaxies Virial mass Epoch of reionization;300 zoom-in simulations; mass-complete sample; Salpeter (1955) IMF.

OBELISKe (Trebitsch et al. 2021) 15 h−1cMpc 40963 DM: 1.2 × 106 M Stars: 1 × 104 M WMAP-7 Galaxy and halo catalogs from Trebitsch et al. (2021) Sum of all DM particles in the main subhalo Epoch of reionization; high-resolution; focused on proto-cluster assembly; re-simulates HORIZON-AGN subvolume; Kroupa (2001) IMF.

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