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Fig. 7.

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Mgas as a function of redshift for different M. The dots represent Mgas estimates from this work using the δ GDR MRZ $ \delta_{\mathrm{GDR}}-\rm MRZ $ method. 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 and thin solid colour lines represent the best-fit from this work, using Eq. (21) and Eq. (20), respectively. The dashed lines are the fits extrapolation. The shaded area the 68% uncertainty of the fit.

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