Table 5.
Averages of supernova explosion parametersa.
| Sample (size) | Mej | EK | M(56Ni) |
|---|---|---|---|
| (M⊙) | (1051 erg) | (M⊙) | |
| Drout et al. 2011 (5) | ... | ... | 0.570(0.541) |
| Cano 2013 (9) | 5.4(3.4) | 12.6(8.9) | 0.299(0.274) |
| Taddia et al. 2015 (4) | 5.4(2.6) | 10.7(9.4) | 1.110(0.580) |
| Lyman et al. 2016 (5) | 3.3(2.7) | 6.1(6.5) | 0.322(0.162) |
| Prentice et al. 2016 (9) | ... | ... | 0.151(0.073) |
| This work (24) | 3.9(2.8) | 7.1(5.7) | 0.309(0.164) |
Notes.
From Arnett semi-analytic models of SNe Ic-BL (not associated with GRBs) from the literature and this work. Uncertainties in the averages are the standard deviations. We removed the GRB SN iPTF13bxl and the peculiar iPTF15eov and iPTF16asu from our sample when computing the average. Prentice et al. (2016) do not include extinction corrections for some SNe Ic-BL.
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