Table E.3.
Arnett model parameters.
SN | Mej | MNi | Ek | texp | Vph |
---|---|---|---|---|---|
(M⊙) | (M⊙) | (1051 erg) | (restframe days) | (km s−1) | |
09dfk | 22.6 ± 1.8 | 0.58 ± 0.01 | 7.3 ± 2.3 | 2.2 ± 0.9 | 7300 ± 1100 |
10inj | 26.4 ± 1.0 | 0.39 ± 0.01 | 16.4 ± 1.7 | 0.0 ± 0.3 | 10200 ± 500 |
11bov | 13.0 ± 1.0 | 0.42 ± 0.02 | 4.6 ± 0.6 | 1.5 ± 0.3 | 7700 ± 400 |
11mnb | 32.4 ± 5.0 | 0.48 ± 0.05 | 5.6 ± 0.9 | −9.3 ± 0.5 | 5400 ± 200 |
11mnb_peak1 | 13.3 ± 2.5 | 0.55 ± 0.03 | 2.3 ± 0.4 | −4.3 ± 5.3 | 5400 ± 200 |
11rka | 20.3 ± 4.0 | 0.54 ± 0.03 | 18.2 ± 3.6 | 7.7 ± 10.2 | 12200 ± 200 |
15dtg | 11.6 ± 0.4 | 0.36 ± 0.01 | 4.0 ± 0.9 | 4.6 ± 0.2 | 7600 ± 900 |
16flq | 10.1 ± 2.6 | 0.23 ± 0.01 | 9.2 ± 2.6 | 11.7 ± 2.3 | 12400 ± 700 |
16hgp | 9.7 ± 0.4 | 0.48 ± 0.01 | 3.2 ± 0.5 | 6.8 ± 0.3 | 7400 ± 600 |
Notes. Arnett model parameters with their statistical fitting uncertainties and measured characteristic ejecta velocities. 11mnb_peak1 refers to the fit to only the first peak of 11mnb. The explosion epochs were fit as described in the text and their shift and uncertainty is listed under the texp column. There is a significant correlation between errors on texp and Mej. MNi could be driven up by host extinction correction, which we do not apply. The distance uncertainty (e.g., random from peculiar velocities or systematic from H0) is not included in the error terms.
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