Table 6
Physical parameters from quasi-bolometric light curves.
| SN | M Ni | M ej | E k |
|
υ ph | log Lmax | t max | Reference |
| [ M⊙ ] | [ M⊙ ] | [ 1051 erg ] |
|
[103 km s-1] | [erg s-1] | [days] | ||
|
|
||||||||
| 2008hw |
|
|
|
|
22 ± 4 | 43.1 ± 0.3 | 12 ± 3 | 1 |
| 2009nz | 0.50 ± 0.04 |
|
|
|
17 ± 1.5 | 43.0 ± 0.2 | 18 ± 4 | 1 |
| 2010ma |
|
|
|
|
22 ± 4 | 43.1 ± 0.2 | 10 ± 2 | 1 |
|
|
||||||||
| 1998bw | 0.38–0.48 | 11 | 50 | 27 | 17 ± 1 | 43.03 ± 0.01 | 17.8 | 2, 3 |
| 0.45 ± 0.01 | 3.4 ± 0.2 | 5.8 ± 1.0 | 6.6 ± 0.4 | 1 | ||||
| 2003dh | 0.25–0.45 | 8 | 40 | 13 | ~ 20 | ~43.0 | ~ 18 | 4 |
| 2003lw | 0.45–0.65 | 13 | 60 | 37 | ~ 18 | ~ 43.2 | ~ 18 | 5 |
| 2006aj | 0.21 | 2 | 2 | 4.0 | 19 ± 1 | 42.99 ± 0.02 | 8.8 | 6, 7 |
| 0.26 ± 0.01 | 0.6 ± 0.04 | 1.3 ± 0.2 | 0.16 ± 0.02 | 1 | ||||
| 2010bh | 0.21 ± 0.03 | 2.6 ± 0.2 | 8.6 ± 2.5 | 2.0 ± 0.8 | 28 | 42.63 | 8.0 | 8, 9 |
|
|
||||||||
| 2002ap | 0.10 | 2.5 | 4 | 3.9 | 14 | ~ 42.4 | ~ 11 | 10 |
| 2003jd | 0.36 | 3 | 7 | 3.9 | 13.5 | ~ 42.9 | ~ 17 | 11 |
| 2007uy | 0.30 ± 0.01 | 4.4 ± 0.3 | 15 ± 1 | 5.6 ± 1.0 | 15.2 | 42.83 | 17.9 | 12 |
| 2008D | 0.07–0.09 | 5.3 ± 1.0 | 6 ± 3 | 25 ± 17 | ~ 10 | ~ 42.4 | ~ 19 | 13, 14 |
| 2009bb | 0.22 ± 0.06 | 4.1 ± 1.9 | 18 ± 7 | 3.8 ± 5.5 | ~ 20 | ~ 42.8 | ~ 18 | 15 |
Notes. Different parts of the table correspond to GRB-SNe analysed here (top), further GRB-SNe (middle), and other SE SNe (bottom). Uncertainties are given at the 1σ level. The υph values correspond to measurements as defined by Eq. (3). The Lmax and tmax values are estimated at the maximum bolometric luminosity, where tmax is defined with respect to the explosion time.
Reference. (1) This paper; (2) Iwamoto et al. (1998); (3) Mazzali et al. (2001); (4) Mazzali et al. (2003); (5) Mazzali et al. (2006b); (6) Pian et al. (2006); (7) Mazzali et al. (2006a); (8) Olivares E. et al. (2012); (9) Bufano et al. (2012); (10) Mazzali et al. (2007); (11) Valenti et al. (2008); (12) Roy et al. (2013); (13) Mazzali et al. (2008); (14) Tanaka et al. (2009); (15) Pignata et al. (2011).
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