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Fig. 6

image

Fit of a hot and a warm BB component to the evolution of the SED of SN 2015da. A warm component dominating at NIR wavelengths is clearly visible from t ≳ +430 d, increasing its strength with time. At t ≳ +730 d a single BB is sufficient to reproduce the SED at IR wavelengths (λ ≳ 1.2 μm).

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