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Fig. 16.

Fig. 16. Refer to the following caption and surrounding text.

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Gas-to-star fractions, μHI (left), μH2 (centre), and Fgas = μH2/(1 + μH2) (right) as functions of Mstar compared to z ≃ 0 observational fits (dotted lines) for main-sequence galaxies (Saintonge et al. 2016, 2017; Tacconi et al. 2018). Different dotted lines in the left panel correspond to fixed Log(SFR/M yr−1) = 0, –1, –2, –3, –4, and –5, from top to bottom. Dashed magenta lines refer to simulation fits (Appendix F, Table F.2).

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