CHARACTERIZING THE<i>V</i>-BAND LIGHT-CURVES OF HYDROGEN-RICH TYPE II SUPERNOVAE

J. P. Anderson, J. E. Thomas-Osip(Las Campanas Observatory), G. Folatelli(Carnegie Observatories), A. Campillay(Las Campanas Observatory), M. Hamuy(University of Chile), F. Olivares(Max Planck Institute for Extraterrestrial Physics), W. Krzemiński(Nicolaus Copernicus Astronomical Center), N. B. Suntzeff(Mitchell Institute), S. González–Gaitán(Universidad de Santiago de Chile), F. Förster(Universidad de Santiago de Chile), L. González(Universidad de Santiago de Chile), J. Maza(Universidad de Santiago de Chile), S. E. Persson(California Institute of Technology), S. Castellón(Las Campanas Observatory), M. Stritzinger, Luis Bolt(University of Bonn), Thomas de Jaeger(Centre National de la Recherche Scientifique), S. Schulze(Northwestern University), C. P. Gutiérrez(University of Turku), N. Morrell(Las Campanas Observatory), M. M. Phillips(Las Campanas Observatory), E. Y. Hsiao(Lawrence Berkeley National Laboratory), K. Krisciunas(Texas A&M University), C. Contreras(Las Campanas Observatory), F. Salgado(Leiden University), Miguel Roth(Las Campanas Observatory), R. Antezana(Universidad de Santiago de Chile), Patrick J. McCarthy(Carnegie Observatories), Wendy L. Freedman(Carnegie Observatories)
The Astrophysical Journal
April 16, 2014
Cited by 376


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