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Fig. 16.

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MOSFiT light curve fits to the first and second peak of SN 2023aew using the different models described in the text. The flat part of the light curve after MJD = 60000 was ignored in the first-peak fit, as the 56Ni model does not include such features. All models have trouble reproducing the simultaneity of the second peak in all optical bands, specifically failing to reproduce the u-band peak, but by eye and by MOSFiT score, the magnetar model provides the best fit.

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