Fig. 6
Comparison of the bolometric light curve (top panel: the shaded area is bounded by the bolometric light curves inferred by Catchpole et al. 1987 and Hamuy et al. 1988) and multi-epoch spectra for SN 1987A and our BSG explosion model Bcl (redshifted and reddened). The label gives the post-explosion epoch and the V -band magnitude offset between model Bcl and SN 1987A.
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