Fig. 20
Revised B12 He4 model bolometric lightcurve with the 56Ni mass increased to 0.075 M⊙ (blue solid line) compared to the pseudo-bolometric UV to MIR lightcurve for SN 2011dh calculated with the spectroscopic method (black dots). For comparison we also show the total γ-ray luminosity corresponding to this amount of 56Ni (black dashed line).
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