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Fig. 5


Bolometric light curves for the grid of magnetar-powered SN models based on the RSG progenitor. The glitch at 125 d occurs when the outer shock with the progenitor wind leaves the Eulerian grid at 1016 cm. In Appendix A, we present light curves for model sets sharing the same Epm or the same Bpm (see Sect. 6 for discussion).

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