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Table 1.

Summary of novelties between M21 and this work.

M21 This Work
Simulation used Single zoom-in galaxy, three snapshots at z ∼ 3, 1728 sightlines each Full SPHINX20 volume in seven snapshots at 4.6 ≤ z ≤ 10 (1380 galaxies total, 10 sightlines each)
Absorption lines C II λ1334 and Si II λ1260 Si II λ1260 and Si II λ1526
Turbulence Fixed vturb = 20 km s−1 (tested 0–50 km s−1) Cell-by-cell turbulence from local velocity gradients (typical 25–100 km s−1)
Dust depletion Neglected Si depletion onto grains included, following De Cia et al. (2016) and Konstantopoulou et al. (2022)
Sub-ionising radiation field UV background from Haardt & Madau (2012) between 6 eV and 13.6 eV Accurate inhomogeneous radiation bins from Katz et al. (2022) restarts
Data output Not published Public dataset of LIS spectra, fesc, and dust attenuation for all galaxies (see Data availability section)

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