Figure 16 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 16.

Fits to the t > 25 days time-integrated bolometric luminosity (bottom) of SNLS05D2bk and SNLS06D1hc with a nickel-powered light curve (dashed lines are for full γ-trapping, visibly different from the solid lines only for SNLS06D1hc). The integrated luminosity is consistent with a nickel decay power source for the light curves, though there are only a few data points and they do not extend to late enough times to make this determination secure. Top plots show the instantaneous luminosity.

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