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Fig. B.1.

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SFR vs molecular gas mass. Different SFR estimates vs MH2: SFR derived from the SED fitting with CIGALE (Nersesian et al. 2019; left panel), and from the hybrid FUV+24μm recipe (Leroy et al. 2019; right panel]). The 85 galaxies are color-coded by their morphological type. The best-fit parameters for each scaling relation are reported in the upper-left corner, while the best-fit line is represented with the black solid line. The intrinsic dispersion (δintr) is reported in the bottom-right corner, followed by the correlation coefficients (namely, P and K).

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