Fig. 5

Bolometric light curves of GRB-SNe, XRF-SNe, and SN 1994I in the corresponding rest frames, dereddened for Galactic extinction. When relevant, a correction for intrinsic extinction was also applied. The curve of SN 2012bz (black points) is from the present work. The others were given by Pian et al. (2006) and Bufano et al. (2012). For clarity, errors in individual datapoints have been reported only for SN 2012bz and SN 2003dh. The model for SN 2012bz (black line) was obtained by scaling down the model of SN 2003dh (red line; Deng et al. 2005) by 15%.
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