Anderson, J. P.; Pessi, Priscila Jael; Dessart, L.; Inserra, C.; Hiramatsu, D.; Taggart, K.; Smartt, S. J.; Leloudas, G.; Chen, T. W.; Möller, A.; Roy, R.; Schulze, S.; Perley, D.; Selsing, J.; Prentice, S.J.; Gal Yam, A.; Angus, C.R.; Arcavi, I.; Ashall, C.; Bulla, M.; Bray, C.; Burke, J.; Callis, E.; Cartier, R.; Chang, S.-W.; Chambers, K.; Clark, P.; Denneau, L.; Dennefeld, M.; Flewelling, H.; Fraser, M.; Galbany, L.; Gromadzki, M.; Gutiérrez, C. P.; Heinze, A.; Hosseinzadeh, G.; Howell, D.A.; Hsiao, E.Y.; Kankare, E.; Kostrzewa-Rutkowska, Z.; Magnier, E.; Maguire, K.; Mazzali, P.; McBrien, O.; McCully, C.; Morrell, Nidia Irene; Lowe, T.B.; Onken, C.A.; Onori, F.; Phillips, M.M.; Rest, A.; Ridden-Harper, R.; Ruiter, A. J.; Sand, D. J.; Smith, K.W.; Smith, M.; Stalder, B.; Stritzinger, M.D.; Sullivan, M.; Tonry, J.L.; Tucker, B.E.; Valenti, S. (EDP Sciences, 2018-12)
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more luminous than normal terminal stellar explosions. The source of the additional power needed to achieve such luminosities is ...