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Fig. B.1.

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Mgas as a function of redshift for different M. The crosses represent Mgas estimates from this work following the method from Scoville et al. (2016). The squares are measurements from Saintonge et al. (2017). The bins that have been corrected for the H-dropout contribution are circled. The thick solid colour lines represent the best-fit from this work using Eq. 20.The shaded area the 68% uncertainty of the fit. The faded solid lines represent the best-fit from this work colour-coded by M (using Eq. 21), the faded dashed lines represent the trend from Tacconi et al. (2018), the faded dotted lines are from Wang et al. (2022).

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