Fig. 14.
Top: attenuation curve slope as a function of the SED continuum amount of attenuation. Middle top: attenuation curve slope versus the stellar mass. Middle bottom: attenuation curve slope versus the SFR. Bottom: attenuation curve slope versus the specific SFR. The blue points correspond to the quantities derived with CIGALE. The black dashed line represents the slope of the mean SMC extinction curve and the yellow dashed line the slope of the Calzetti law. The grey dash-dotted line illustrates the best fit using an orthogonal distance regression (using SciPy’s scipy.odr). The χ2, number of degrees of freedom and Null Hypothesis Probability (NHP) of these fits are indicated.
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