Fig. 5
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R-band light curves for model s15p2NoPwr and s15p2Pwr1e40 compared with a set of observations (for a few objects, we show the r-band magnitude instead; see Table 2). All light curves are shifted so that the magnitude is zero at the onset of the nebular phase (when the fall from the plateau stops and the SN initially follows the rate of 56Co decay).
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