SN 2012fr: Ultraviolet, Optical, and Near-Infrared Light Curves of a Type Ia Supernova Observed Within a Day of Explosion

Carlos Contreras, M. M. Phillips, Christopher R. Burns, Anthony L. Piro, B. J. Shappee, Maximilian D. Stritzinger, C. Baltay, Peter J. Brown, Emmanuel Conseil, Alain Klotz, Peter E. Nugent, Damien Turpin, Stu Parker, D. Rabinowitz, Eric Y. Hsiao, Nidia Morrell, Abdo Campillay, Sergio Castellón, Carlos Corco, Consuelo González, Kevin Krisciunas, Jacqueline Serón, Brad E. Tucker, E. S. Walker, E. Baron, C. Cain, Michael J. Childress, Gastón Folatelli, Wendy L. Freedman, Mario Hamuy, P. Hoeflich, S. E. Persson, Richard Scalzo, Brian Schmidt, Nicholas B. Suntzeff

Published 2018-03-27, updated 2018-04-13Version 3

We present detailed ultraviolet, optical and near-infrared light curves of the Type Ia supernova (SN) 2012fr, which exploded in the Fornax cluster member NGC 1365. These precise high-cadence light curves provide a dense coverage of the flux evolution from $-$12 to $+$140 days with respect to the epoch of $B$-band maximum (\tmax). Supplementary imaging at the earliest epochs reveals an initial slow, nearly linear rise in luminosity with a duration of $\sim$2.5 days, followed by a faster rising phase that is well reproduced by an explosion model with a moderate amount of $^{56}$Ni mixing in the ejecta. From an analysis of the light curves, we conclude: $(i)$ explosion occurred $< 22$ hours before the first detection of the supernova, $(ii)$ the rise time to peak bolometric ($\lambda > 1800 $\AA) luminosity was $16.5 \pm 0.6$ days, $(iii)$ the supernova suffered little or no host-galaxy dust reddening, $(iv)$ the peak luminosity in both the optical and near-infrared was consistent with the bright end of normal Type Ia diversity, and $(v)$ $0.60 \pm 0.15 M_{\odot}$ of $^{56}$Ni was synthesized in the explosion. Despite its normal luminosity, SN 2012fr displayed unusually prevalent high-velocity \ion{Ca}{2} and \ion{Si}{2} absorption features, and a nearly constant photospheric velocity of the \ion{Si}{2} $\lambda$6355 line at $\sim$12,000 \kms\ beginning $\sim$5 days before \tmax. Other peculiarities in the early phase photometry and the spectral evolution are highlighted. SN 2012fr also adds to a growing number of Type Ia supernovae hosted by galaxies with direct Cepheid distance measurements.