Fig. B.2.
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Comparison in the SN IIn model at 300 d of the Hα profile between the MC code and CMF_FLUX when we assume isotropic scattering. All three profiles show similar agreement to that obtained in the absence of dust (see Fig. B.1). The red component of the CMF calculation (i.e., obs_cmf) shows some rounding due to numerical diffusion in frequency space.
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