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Fig. 4


Distribution of ALLSMOG galaxies as a function of M (upper-left), SFR (upper-right), SSFR (bottom-left) and redshift (bottom-right). The full sample is represented by the coloured histogram, and the hatched histogram traces the non-detections. At the bottom of each histogram we show the corresponding detection fraction per bin, computed as the ratio between the number of sources detected in CO and the number of sources observed in that bin.

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