Distribution of the rise time to maximum (tpeak) and bolometric luminosity at maximum (Lpeak) for a range of magnetar field strengths and initial spin periods (the ejecta mass is 5 M⊙, the ejecta kinetic energy is 1051 erg, and the adopted opacity is 0.2 cm2 g−1). The figure is adapted from Kasen & Bildsten (2010), using their Eqs. (15) and (16).
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