Fig. 10
Left panel: relation between the specific star formation rate and the gas fraction in three classes of increasing DefHI, excluding objects fainter than M∗ = 109M⊙. Right panel: same as in the left panel, but including fainter objects. The histograms drawn on top and to the right show the counts of galaxies with given HI gas fraction and SSFR, with the mean values given in three bins of DefHI.
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