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Table A.3.
56Ni mass estimates for SN 2022lxg.
| Method | Value |
| Arnett, peak, Stf-Bol | 1.210± 0.160 M⊙ |
| Arnett, Tail, Stf-Bol | 0.008± 0.003 M⊙ |
| Hamuy, tail, Stf-Bol | 0.002± 0.001 M⊙ |
| 1987A, tail, Stf-Bol | 0.009± 0.004 M⊙ |
| Arnett, peak, pseudo-bol | 0.247± 0.003 M⊙ |
| Arnett, Tail, pseudo-bol | 0.002± 0.001 M⊙ |
| Hamuy, tail, pseudo-bol | < 0.001 M⊙ |
| 1987A, tail, pseudo-bol | 0.003± 0.001 M⊙ |
Notes. We derive the peak and the tail 56Ni mass estimates from the luminosities calculated with two different methods, either from the blackbody fits and the Stefan-Boltzmann law, or from the pseudo-bolometric luminosity estimates (see Sect. 3.2.2 for details).
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