M∗-independent quantity as a function of Hi gas mass for the sample of galaxies shown in Fig. 11. As explained in the caption of Fig. 11, the COLD GASS galaxies with a non detection in Hi are not shown in this plot, because upper limits on MHI are not available for these sources. For an explanation of the symbols and lines drawn on the plot, we refer to the caption of Fig. 8. The results of the regression analysis are reported in Table A.1. As for the relation shown in Fig. 11, the analysis was performed by including only the detections in Hi.
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