Fig. 11
Piro & Nakar (2013) model (dashed lines) for the early light curve of iPTF15dtg, in Bgri-bands. In the modeling, we adopt the ejecta mass and explosion energy derived from the hydrodynamical modeling. The large ejecta mass implies a long timescale for the cooling tail in the optical, which cannot reproduce the early peak of iPTF15dtg.
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