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Fig. 4.


Variation of the median effective attenuation curves with AFUV (color coded). We only select here galaxies with a disk inclination between 30° and 50°. The median trend of the full sample is plotted with the solid gray line. We compare this trend to a set of standard attenuation curves, Calzetti et al. (2000): circles, Reddy et al. (2016): squares and Gordon et al. (2003; SMC): triangles.

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