Distribution of the ALLSMOG sample as a function of the Hi gas mass. As in Figs. 4–6, the coloured histogram indicates the full sample, and the hatched histogram traces the non-detections. The detection fraction per MHI bin is shown at the bottom of the histogram. Galaxies for which we have only an upper limit on MHI are not included in this plot (see Sect. 4.2 and Table C.5). We use the MHI values corrected for self-absorption.
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