SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event
G. Dimitriadis(Trinity College Dublin), D. R. Young(Queen's University Belfast), K. Maguire(University of Oxford), Ryan J. Lebron, L. Galbany, Alexandra Kozyreva(Heidelberg Institute for Theoretical Studies), M. Gromadzki(Astronomical Observatory), T. E. Müller-Bravo(Trinity College), Adam A. Miller(University of California, Berkeley), J. Sollerman(Stockholm University), M. Della Valle(Centre National de la Recherche Scientifique), Ryan Ridden-Harper(Johns Hopkins University), A. J. Drake(California Institute of Technology), K. Taggart(University of California, Santa Cruz), M. W. Coughlin(University of Minnesota), S. Schulze(Northwestern University), Abigail Polin(California Institute of Technology), C. P. Gutiérrez(University of Turku), N. Ihanec(European Southern Observatory), M. Nicholl(Queen's University Belfast), Viraj Karambelkar, Steven L. Groom(California Institute of Technology), J. Johansson(Stockholm University), B. Rusholme(California Institute of Technology), C. Inserra(Cardiff University), Shubham Srivastav(Queen's University Belfast), Chang Liu(Northwestern University), Yi Yang, Qinan Wang(Johns Hopkins University), T. W. Chen(National Central University), J. P. Anderson
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