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Fig. 22


Luminosity in Mg I] λ4571 (left) and Mg I λ1.504 μm (right) relative to the 56Co decay power in SN 1993J, SN 2008ax, and SN 2011dh, and in the models. The Mg I] λ4571 line is typically very blended in the models before 300 days, and so we do not plot the output of the line extraction algorithm before this time.

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