The Observer’s Guide to the Gamma-Ray Burst Supernova Connection

Figure 9

Bolometric LCs of a sample of GRB-SNe. Times are given in the rest-frame. The average peak luminosity of all GRB-SNe except SN 2011kl is  erg , with a standard deviation of  erg . The peak luminosity of SN 2011kl is  erg , which makes it more than 5 more luminous than the average GRB-SN. The average peak time of the entire sample is  d, with a standard deviation of 2.6 d. If SN 2011kl is excluded from the sample, this changes to 13.0 d. Plotted for reference is an analytical model that considers the luminosity produced by the average GRB-SN ( erg,  , and  ).