Fig. 10.
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Cold gas fractions (left panel) and depletion times (right panel) in star-forming galaxies in the DIANOGA PCs (orange) and in the cosmological box (green) as a function of stellar masses. Solid lines (shaded regions) show median values (16th–84th percentile ranges, respectively). For comparison, we show observations at z ∼ 1.5 − 3 from Magdis et al. (2012), Liu et al. (2019), Sanders et al. (2023), Mérida et al. (2024) and Leroy et al. (2024).
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