Fig. 1.
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Bolometric light curves for the models P250Ni25 (red curve, labelled ‘Ni25’), P250Ni34 (blue curve, labelled ‘Ni34’), and P250Ni34mix (cyan curve, labelled ‘Ni34mix’), and the bolometric light curve for SLSN 2018ibb (grey curve, labelled ‘2018ibb’) taken from Schulze et al. (2024). Time ‘0’ corresponds to the peak in g and r-band magnitude, similar to the tmax in Schulze et al. (2024).
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