A radio-detected type Ia supernova with helium-rich circumstellar material
Erik C. Kool(Stockholm University), Daniel Stern(Jet Propulsion Laboratory), Takashi J. Moriya(Kavli Institute for the Physics and Mathematics of the Universe), Jeremy Lezmy(Lyon 1 Université), Kishalay De(California Institute of Technology), J. Sollerman(Stockholm University), S. Yang(Stockholm University), M. Á. Pérez-Torres(Consejo Superior de Investigaciones Científicas), M. J. Graham, Y. Sharma(California Institute of Technology), Frank J. Masci, S. Mattila, Josiah Purdum, C. Fremling(California Institute of Technology), Peter Lundqvist(AlbaNova), S. D. Ryder(Australian National University), A. Gal‐Yam(Weizmann Institute of Science), T. Reynolds(University of Turku), Michael S. Medford(Lawrence Berkeley National Laboratory), D. A. Perley(Liverpool John Moores University), J. S. Bloom(University of California, Berkeley), Igor Andreoni(University of North Carolina at Chapel Hill), S. Schulze(Northwestern University), Laura Chomiuk, Eric C. Bellm(University of Washington), Conor M. B. Omand(Stockholm University), Chelsea Harris(Michigan State University), Estelle Robert(Lyon 1 Université), Steven L. Groom(California Institute of Technology), J. Johansson(Stockholm University), Sungmin Park(Ulsan National Institute of Science and Technology), M. M. Kasliwal(California Institute of Technology), J. Moldón(Consejo Superior de Investigaciones Científicas), Mathew Smith(Institute of Nuclear Physics of Lyon), Reed Riddle, N. L. Strotjohann(Weizmann Institute of Science), K. Maguire(University of Oxford)
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