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Fig. 5

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LCs of SN 1054 and our ecSNe exploded within super-AGB winds. The V-band LCs of the models are shown. The observations of SN 1054 are based on human eyes, which are sensitive at around the V band (Vos 1978). Note that the V-band and R-band magnitudes are similar in our models (Fig. 3).

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