Table 2
GRBs–SNe properties.
| GRB – SN | z | E γ,iso | M bol | Refs. |
|
|
||||
| (× 1052 erg) | ||||
|
|
||||
| 980425 – 1998bw | 0.0085 | 0.00010 ± 0.00002 | −18.65 ± 0.20 | 1, 2 |
| 030329 – 2003dh | 0.1687 | 1.5 ± 0.3 | −18.71 ± 0.15 | 3,4 |
| 031203 – 2003lw | 0.1055 | 0.010 ± 0.004 | −18.92 ± 0.20 | 5, 1 |
| 060218 – 2006aj | 0.0334 | 0.0053 ± 0.0003 | −18.16 ± 0.20 | 4, 6, 7 |
| 100316D – 2010bh | 0.0591 | 0.007 ± 0.003 | −17.50 ± 0.25 | 8, 9 |
| 120422A – 2012bz | 0.283 | 0.024 ± 0.008 | −18.56 ± 0.15 | 10 |
| 130427A – 2013cq | 0.3399 | 81.0 ± 8.0 | −18.91 ± 0.20 | 11, 2 |
| 130702A – 2013dx | 0.145 | 0.065 ± 0.010 | −18.51 ± 0.15 | 12, 13 |
Notes. Columns: (1) GRB–SN name, (2) redshift, (3) isotropic γ-ray energy in the 1−10 000 keV energy band, and (4) peak bolometric magnitude of the SN.
Reference. 1) Amati et al. (2006); 2) this work; 3) Deng et al. (2005); 4) Amati et al. (2008); 5) Mazzali et al. (2006a); 6) Pian et al. (2006); 7) Ferrero et al. (2006); 8) Bufano et al. (2012); 9) Starling et al. (2011); 10) Melandri et al. (2012); 11) Maselli et al. 2014; 12) D’Elia et al. (in prep.); 13) Amati et al. (2013b; note that uncertainty on Eγ,iso is amended here).
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