Table D.1.
‘Best-fit’ model according to different statistical estimators and flux scales.
Flux scale | MAD | MFE | MADlog | MFElog | Score |
---|---|---|---|---|---|
Fν | GCD | GCD | MERGER | MERGER | MERGER |
Fν, norm | GCD | GCD | MERGER | MERGER | MERGER |
![]() |
GCD | GCD | MERGER | MERGER | MERGER |
![]() |
GCD | GCD | MERGER | GCD | MERGER |
Fλ | DDT | DBLEDET | DBLEDET | DBLEDET | DBLEDET |
Fλ, norm | DDT | GCD | MERGER | MERGER | MERGER |
![]() |
DDT | DBLEDET | DBLEDET | DBLEDET | DBLEDET |
![]() |
MERGER | GCD | MERGER | MERGER | MERGER |
Notes: The ‘norm’ subscript indicates the model fluxes have been normalised to the mean observed flux over the full 0.35–14 μm range, while the ‘red’ superscript indicates the observed SN 2021aefx spectrum was not corrected for extinction by dust in the host galaxy (i.e. the spectra become redder).
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