The broad-lined Type-Ic supernova SN 2022xxf and its extraordinary two-humped light curves - I. Signatures of H/He-free interaction in the first four months

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Fig. A.1

Bolometric light curves of SN 2022xxf (red points) and SN 1998bw (Patat et al. 2001; Clocchiatti et al. 2011) (blue points; light blue for the scaled-down LC). Solid lines are spline representations of the LCs. The difference between the LC of SN 2022xxf and the scaled-down LC of SN 1998bw is plotted with a dashed orange line. The dotted gray lines indicate ⁵⁶Ni fits using HAFFET.

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