Fig. 7.
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Molecular masses derived for the CO-ARC sample. Detection are shown with filled circles and upper limits are indicated with open circles and arrows. For comparison, we show the predicted evolution of the molecular gas content with redshift from semi-empirical models of normal star-forming galaxies with halo masses of Mvir = 1013 and Mvir = 1014 (Popping et al. 2015).
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