On the diversity of superluminous supernovae: ejected mass as the dominant factor
M. Nicholl(Queen's University Belfast), F. Yuan(Australian National University), M. Fraser(University of Cambridge), S. Baumont(Centre National de la Recherche Scientifique), K. Maguire(University of Oxford), L. Galbany, D. Rabinowitz(Yale University), B. Schmidt(Australian National University), F. E. Bauer(Space Science Institute), J. Sollerman(Stockholm University), M. T. Botticella(Astronomical Observatory of Capodimonte), D. R. Young(Queen's University Belfast), L. Le Guillou(Laboratoire de Physique Nucléaire et de Hautes Énergies), Anders Jerkstrand(Queen's University Belfast), S. Benetti(Osservatorio Astronomico di Padova), F. Taddia(Stockholm University), M. Della Valle(Centre National de la Recherche Scientifique), C. Baltay(Yale University), U. Feindt(Stockholm University), A. Gal‐Yam(Weizmann Institute of Science), D. Bersier(Unknown), S. Valenti(Osservatorio Astronomico di Padova), J. Polshaw(Queen's University Belfast), M. Dennefeld(Centre National de la Recherche Scientifique), S. Rostami(Yale University), S. Schulze(Northwestern University), S. J. Smartt(University of Oxford), E. Hadjiyska(Yale University), G. Leloudas(University of Copenhagen), N. Elias–Rosa(Institute of Space Sciences), P. A. Mazzali(Tokyo University of Science), R. Scalzo(Australian National University), R. McKinnon(Yale University), K. Smith(Queen's University Belfast), C. Inserra(Cardiff University), M. Sullivan(University of Oxford), T. W. Chen(National Central University), E. Kankare(Queen's University Belfast), M. Childress(Australian National University), Stuart Sim(Queen's University Belfast)
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