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Table C.1.
Supernova model fitting priors.
| Prior | default | magni | csmni |
|---|---|---|---|
| κγ [cm2 g−1] | 2.70 × 10−2 | 2.70 × 10−2 | 2.70 × 10−2a |
| Ekin [1051 erg] | − | − | log([10−1, 102])b |
| s | − | − | [0.00, 2.00] |
| ρ [g cm3] | − | − | log([10−15, 10−11]) |
| T [K] | log([3.00 × 103, 104]) | log([3.00 × 103, 104]) | log([103, 105]) |
| Mej [M⊙] | [10−1, 102] | [10−1, 102] | [10−1, 2.00 × 102] |
| κ [cm2 g−1] | [5.00 × 10−2, 3.40 × 10−1] | [5.00 × 10−2, 3.40 × 10−1] | [5.00 × 10−2, 3.40 × 10−1]c |
| σ | log([10−3, 102]) | log([10−3, 102]) | log([10−5, 101]) |
| MCSM [M⊙] | − | − | [10−1, 2.00 × 102] |
| fNi | [10−2, 5.00 × 10−1] | [10−2, 5.00 × 10−1]d | [10−2, 5.00 × 10−1]e |
| r0 [AU] | − | − | log([10−2, 102]) |
| MNS [M⊙] | − | [1.50, 1.90] | − |
| vej [km s−1] | [103, 105] | [103, 105] | −f |
| Bfield [1014 G] | − | [10−1, 1.50 × 101] | − |
| δ | − | − | 0.00 |
| Pspin [ms] | − | [7.00 × 10−1, 101] | − |
| θPB [radians] | − | [0.00, 1.57] | − |
| n | − | − | [7.00, 1.20 × 101] |
Notes. aκγ was not specified in csmbTo get this range of Ekin, we set Mej ∈ [0.1, 200] M⊙ and vej ∈ log([103, 105]) km s−1cκ was not specified in csmdThe magnetar model does not use fNieThe csm model does not use fNifvej in csmni is already embedded in Ekin.
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