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Caption: Fig. 3.
The quantity ﹩d\sigma _{\mathrm{sca}\,}/ d\Omega ﹩ at selected wavelengths λ as a function of the scattering angle θ for WD01 models for Milky Way dust with ﹩R_{V}=3.1﹩, LMC average dust, and SMC bar dust. Curves are labeled by wavelength λ.
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