Figure 15 from RAPIDLY RISING TRANSIENTS IN THE SUPERNOVA

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RAPIDLY RISING TRANSIENTS IN THE SUPERNOVA—SUPERLUMINOUS SUPERNOVA GAP

Authors: Iair Arcavi, William M. Wolf, D. Andrew Howell, Lars Bildsten, Giorgos Leloudas, Delphine Hardin, Szymon Prajs, Daniel A. Perley, Gilad Svirski, Avishay Gal-Yam, Boaz Katz, Curtis McCully, S. Bradley Cenko, Chris Lidman, Mark Sullivan, Stefano Valenti, Pierre Astier, Cristophe Balland, Ray G. Carlberg, Alex Conley, Dominique Fouchez, Julien Guy, Reynald Pain, Nathalie Palanque-Delabrouille, Kathy Perrett, Chris J. Pritchet, Nicolas Regnault, James Rich, and Vanina Ruhlmann-Kleider

2016 The Astrophysical Journal 819 35.

Provider: AAS Journals

Caption: Figure 15.

Two of the closest fits between white dwarf detonation models and our light curves. Top: SNLS04D4ec compared to the Sim et al. (2010) 1.15M_⊙ model. Bottom: SNLS05D2bk compared to the Kromer et al. (2010) model number 6. Both SNe do not trace the model post-peak declines or their color evolution. The other models from the Sim et al. (2010) and Kromer et al. (2010) sets were even further from the data and none were able to reasonably fit SNLS06D1hc at any phase.

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