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Fig. C.1.

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Molecular gas fraction, fmolgas, (Equation C.3) as a function of stellar mass as inferred from the Band-7 dust continuum based on Equation C.1. The points are colour-coded by their classifications described in Section 3. The empty circles represent upper limits. The median gas fraction of the CRISTAL sample is ∼ 0.5. Our measurements are in broad agreement with those reported by Dessauges-Zavadsky et al. (2020) for the ALPINE samples (purple hexagons), in which we both observe a similar slope of dependence of fmolgas on M, similar to that of the lower redshifts 1≲ z ≲6 star-forming galaxies compiled by Dessauges-Zavadsky et al. (2020) and references therein (light grey to blue markers).

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