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Table 3.
Priors and posterior of the parameters fit with REDBACK for the generalized magnetar model.
Parameters | Priors | Best-fit values | Best-fit values |
---|---|---|---|
SN 2020xga | SN 2022xgc | ||
Initial magnetar spin-down luminosity L0 (erg s−1) | ℒ (1040, 1050) |
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Magnetar spin-down time tSD (s) | ℒ (102, 108) |
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Magnetar braking index n | 𝒰 (1.5, 10) |
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Ejecta nickel mass fraction f56Ni | ℒ (10−6, 1) |
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Ejecta mass Mej (M⊙) | 𝒰 (0.1, 100) |
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Supernova explosion energy ESN (erg) | 𝒰 (5 × 1049, 3 × 1051) |
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Ejecta gamma-ray opacity κγ (cm2 g−1) | ℒ (10−4, 104) |
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Photospheric plateau temperature Tfloor (K) | 𝒰 (3 × 103, 2 × 104) |
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Explosion date texp (MJD) | 𝒰 (FD − 100, FD − 0.1) |
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Notes. The 𝒰 stands for uniform, and ℒ for log-uniform. The FD acronym stands for first detection and represents the date of the first real detection. The uncertainties are reported at 1σ significance.
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