Fig. 3.
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Evolution of some spectral properties for model s15p2 over the time span from 200 to 500 d after explosion. We show the evolution of the cumulative flux integrated from 0.1 to 30.0 μm (left) and the evolution of the percentage, fractional luminosity relative to the bolometric luminosity of a few strong lines in the infrared (right). (See Section 3 for discussion.)
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