The lowest metallicity type II supernova from the highest mass red-supergiant progenitor
J. P. Anderson, S. Valenti(Osservatorio Astronomico di Padova), M. Fraser(University of Cambridge), K. Maguire(University of Oxford), L. Galbany, T. Lowe(University of Hawaii System), S. González–Gaitán(Universidad de Santiago de Chile), J. Sollerman(Stockholm University), D. R. Young(Queen's University Belfast), Anders Jerkstrand(Queen's University Belfast), C. Agliozzo(Universidad Andrés Bello), G. Hosseinzadeh(University of Arizona), M. E. Huber(Technical University of Munich), S. Mattila, S. Castellón(Las Campanas Observatory), M. Stritzinger, H. Flewelling(University of Hawaiʻi at Mānoa), S. J. Smartt(University of Oxford), K. C. Chambers(University of Hawaii System), C. P. Gutiérrez(University of Turku), N. Morrell(Las Campanas Observatory), M. M. Phillips(Las Campanas Observatory), C. González(Las Campanas Observatory), Luc Dessart(Centre National de la Recherche Scientifique), E. Y. Hsiao(Lawrence Berkeley National Laboratory), C. Inserra(Cardiff University), M. Sullivan(University of Oxford), T. W. Chen(National Central University), C. Contreras(Las Campanas Observatory), E. Kankare(Queen's University Belfast), T. Krühler(Max Planck Institute for Extraterrestrial Physics), E. A. Magnier(University of Hawaii System)
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