Summary of the four GRB events studied here.
|SN||SN 2012eb||SN 2013fu|
|T90 (s)||15 ± 2||101.2 ± 5.4||159 ± 34||32.5 ± 2.5|
|log Eγ, iso|
|log Lγ, iso|
Notes. Burst durations are given in the observer frame and were taken from http://swift.gsfc.nasa.gov/archive/grb_table/. The isotropic-equivalent energies (in units of erg) were derived from the observed high-energy properties (Briggs & Younes 2011; Golenetskii et al. 2013), and using the statistically inferred high-energy properties of GRBs (Butler et al. 2007). Lγ, iso is the time-averaged luminosity (erg s−1) of the burst, here defined as Eiso/T90. References for the redshifts are given in Appendix A.
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