Fig. 6.
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Results of the BB fitting. Top: bolometric LC of SN 2021efd (black) and bolometric luminosity of Type Ib SN 2004gv (blue) (Taddia et al. 2018) indicated by a dotted blue line. Middle: BB temperature of the photosphere. Bottom: BB radius of the photosphere. The errors are the 1σ uncertainties of the χ2-fitting. Since the cadence after 115 days is poor, these observations were plotted separately.
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