Fig. 8.
Magnetar-powered SN model for OGLE14-073. The SN is assumed to have exploded texp = 20 days before discovery. The points show the bolometric luminosities (upper panel) and Fe II velocities (lower panel) from observations published by Terreran et al. (2017). The model is shown with solid lines and the parameters used in the simulation are presented in Table 2.
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