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Caption: Fig. 4.
Extinction cross section per H, albedo, ﹩\langle \mathrm{cos}\,\rangle ﹩, and ﹩\langle \mathrm{\cos}^{2}\rangle ﹩ calculated for WD01 models for Milky Way dust with ﹩R_{V}=3.1﹩, 4.0, and 5.5, average LMC dust, and dust in the SMC bar.
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