Table 4
56Ni mass fit results for different explosion models, as described in detail by The & Burrows (2014).
100 keV band | 20 keV band | ||||||||
|
|||||||||
Rank | Model | χ 2 | M(56Ni) | Model | χ 2 | M(56Ni) | Model | χ 2 | M(56Ni) |
|
|||||||||
1. | hed8 | 25.07 | 0.46 ± 0.06 | hed8 | 7.81 | 0.52 ± 0.12 | W7 | 16.98 | 0.42 ± 0.07 |
2. | w7dt | 25.37 | 0.50 ± 0.06 | w7dt | 7.89 | 0.57 ± 0.13 | det2 | 17.07 | 0.38 ± 0.06 |
3. | W7A | 25.57 | 0.51 ± 0.06 | W7A | 7.95 | 0.59 ± 0.13 | m36 | 17.15 | 0.43 ± 0.07 |
4. | hecd | 25.61 | 0.52 ± 0.06 | hecd | 8.11 | 0.58 ± 0.13 | dd202c | 17.26 | 0.42 ± 0.07 |
5. | hed6 | 26.22 | 0.50 ± 0.06 | hed6 | 8.54 | 0.56 ± 0.13 | W7E | 17.29 | 0.43 ± 0.07 |
6. | det2 | 27.84 | 0.50 ± 0.06 | det2 | 9.35 | 0.55 ± 0.13 | dd4 | 17.33 | 0.45 ± 0.07 |
7. | w7dn | 28.27 | 0.54 ± 0.07 | w7dn | 9.57 | 0.59 ± 0.14 | w7dn | 17.33 | 0.40 ± 0.06 |
8. | W7E | 29.48 | 0.56 ± 0.07 | W7E | 10.11 | 0.61 ± 0.15 | det2e2 | 17.67 | 0.44 ± 0.07 |
9. | m36 | 30.30 | 0.56 ± 0.07 | m36 | 10.44 | 0.61 ± 0.15 | hed6 | 17.73 | 0.37 ± 0.06 |
10. | W7 | 30.52 | 0.54 ± 0.07 | W7 | 10.50 | 0.59 ± 0.14 | hecd | 18.13 | 0.38 ± 0.06 |
11. | dd202c | 30.70 | 0.55 ± 0.07 | dd202c | 10.51 | 0.61 ± 0.15 | hed8c | 18.17 | 0.33 ± 0.05 |
12. | dd4 | 32.72 | 0.57 ± 0.08 | dd4 | 11.35 | 0.62 ± 0.15 | w7dt | 18.33 | 0.36 ± 0.06 |
13. | det2e2 | 34.18 | 0.56 ± 0.07 | det2e2 | 11.80 | 0.61 ± 0.15 | W7A | 18.40 | 0.38 ± 0.06 |
14. | pdd54 | 38.84 | 0.56 ± 0.08 | pdd54 | 13.52 | 0.61 ± 0.16 | pdd14 | 18.74 | 0.46 ± 0.07 |
15. | det2e6 | 50.75 | 0.72 ± 0.11 | det2e6 | 17.80 | 0.78 ± 0.25 | det2e6 | 22.94 | 0.66 ± 0.11 |
constant | 35.20 | 0.30 ± 0.06 | constant | 8.48 | 0.41 ± 0.12 | constant | 26.86 | 0.24 ± 0.06 | |
bgd only | 90.92 | – | bgd only | 27.87 | – | bgd only | 57.33 | – |
Notes. We fit the light curves resulting from those models to our gamma-ray data. The fit quality can be seen from the χ2 values (for 9 degrees of freedom, except for the bgd-only case which has 10 d.o.f.). Fitted 56Ni masses are given in M⊙ with uncertainties, for the intensity variation time profile of the respective model. We compare results for three analysis approaches, fitting a single broad line (left), for taking the non-zero flux in a broad band (middle) (800–900 keV), and for taking nonzero flux in a band where the 56Co emission could be expected to appear (right) (840–860 keV).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.