Fig. 5.
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Simulated light-curves for a magnetar with a dipolar magnetic field of 1014 G (panel a), 1015 G (panel b), and 1016 G (panel c) assuming the DD2 EoS with a 2.37 M⊙ NS mass. The top panels show the emission from the two considered viewing angles, and the bottom panels detail the physical origins of the emission. Times are measured relative from merger.
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