Fig. 4
Dust attenuation curve as derived from our radiative transfer calculations (triple dotted-dashed purple line). The dust extinction curves derived for the Milky Way with RV = 3.0 (Fitzpatrick & Massa 2007) and the Small Magellanic Clouds (Gordon et al. 2003), and the Calzetti et al. (1994) attenuation law for starburst galaxies are added for comparison as black solid, red dotted-dashed and green dashed lines, respectively.
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