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Fig. 3.

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Light curves of SN 2019jrj computed in the 4000–7000 Å range under the assumptions that a jet break occurs at 7 rest-frame days or does not occur until at least several months after the GRB. The light curves of other core-collapse SNe computed in the same wavelength range from available photometry (Galama et al. 1998; McKenzie & Schaefer 1999; Patat et al. 2001; D’Elia et al. 2015; Toy et al. 2016; Mazzali et al. 2021; Pian et al. 2006; Ferrero et al. 2006; Taubenberger et al. 2006; Foley et al. 2003; Tomita et al. 2006) are shown, as is the light curve of SN 1998bw in the 3000–10 000 Å range (dotted red curve). For clarity, uncertainties are shown only for SN 2019jrj.

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