Multi-band light curves (left) and multi-epoch spectra (right) for the He-giant star explosion model He_R173 (solid) and the observations (symbols) of SN 2008D. The time sequence is computed between 1 d and 7 d after explosion. In this figure, we either correct the model or the observations for distance, reddening, and redshift of SN 2008D (see Sect. 2 for details).
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