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Fig. 9.


Bolometric luminosity of the 17 GRB SNe according to Table 2. In addition we show the bolometric light curve of SN 1998bw (in black), which we took from Greiner et al. (2015; their Fig. 3) and performed a smoothed spline fit. All other SN light curves were then scaled accordingly using the corresponding bolometric values for the stretch and luminosity factor (Eq. (1)). The four GRB SNe discussed here are drawn in brown. We note that this plot is a visualization of the (sbol, kbol) values in Table 2 and is not based on individual data points.

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