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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.