Fig. 2.
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Light curve of SN 2016jbu including HST observations from Table 1 and Brennan et al. (2022b), and V-band (black markers) observations from Brennan et al. (2022a). We include the expected luminosity from 0.016 M⊙ of 56Ni in the V-band (Hamuy 2003; Brennan et al. 2022b) as the sloped dashed line. We connect points in the late-time light curve to visualise the non-linear decline.
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