Fig. 10

Best fits to the bolometric light curve of OGLE-2014-SN-131 for three different models. The dashed red line shows the simple Arnett (radioactive decay) model, the dashed blue line shows the best magnetar model, the dashed green line indicates the best CSM interaction model, and finally, the dashed gray line is an alternative radioactive decay model with recombination. The radioactive decay models cannot reproduce the relatively fast decline of the light curve.
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