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Fig. 3


Upper limits on the luminosity of SN2013fc from the individual analysis of the 2-year time window. Down arrows indicate upper limits at 2σ confidence.The black line represents the integrated luminosity computed from a simulated spectrum derived by Murase et al. (2015) for a neutron star with P = 10 ms, B = 1013 G at a distanced = 16.5 kpc and about 206 days after explosion.

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