M∗-independent quantity as a function of nebular visual extinction for the sample of local star-forming galaxies defined by the ALLSMOG survey and by the sub-sample of COLD GASS selected in Sect. 5. The top and bottom plots were produced by using the AV values obtained by employing the Cardelli et al. (1989)’s and Calzetti et al. (2000)’s attenuation curves, respectively. We refer to the caption of Fig. 8 for an explanation of the symbols and lines shown in the plot. The results of the regression analysis are reported in Table A.1. As for the relations in Fig. 9, the fit was performed without accounting for the measurement error on AV (of the order of ~ 0.5 mag).
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