Fig. A.1.
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Molecular gas fraction fmol = Mmol/SFR vs. stellar mass for main sequence galaxies according to the definitions of Renzini & Peng (2015) (top) and Saintonge & Catinella (2022) (bottom), respectively. The black diamonds correspond to the binned medians computed using the Kaplan-Meier estimator. Open symbols with downward arrows denote upper limits. The associated error bars show the extent of the bin (in x) and the 25–75 percentile interval (in y)
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