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Nicholl, M.Smartt, S. J.Jerkstrand, A.Inserra, C.Sim, S. A.Chen, T. W.Benetti, S.Fraser, M.Gal Yam, AvishayKankare, E.Maguire, K.Smith, K.Sullivan, M.Valenti, S.Young, D. R.Baltay, C.Bauer, F. E.Baumont, S.Bersier, D.Botticella, M. T.Childress, M.Dennefeld, M.Della Valle, MassimoElias Rosa, N.Feindt, U.Galbany, LluisHadjiyska, E.Le Guillou, L.Leloudas, G.Mazzali, P.McKinnon, R.Polshaw, J.Rabinowitz, D.Rostami, S.Scalzo, R.Schmidt, B. P.Schulze, S.Sollerman, J.Taddia, F.Yuan, F.[On the diversity of superluminous supernovae: ejected mass as the dominant factor]

Smartt, S. J.Valenti, S.Fraser, M.Inserra, C.Young, D. R.Sullivan, M.Pastorello, A.Benetti, S.Gal-Yam, A.Knapic, C.Molinaro, M.Smareglia, R.Smith, K.W.Taubenberger, S.Yaron, O.Anderson, J. P.Ashall, C.Balland, C.Baltay, C.Barbarino, C.Bauer, Franz ErikBaumont, S.Bersier, D.Blagorodnova, N.Bongard, S.Botticella, M.-T.Bufano, F.Bulla, M.Cappellaro, E.Campbell, H.Cellier Holzem, F.Chen, T. W.Childress, M. J.Clocchiatti, A.Contreras, C.Dall’Ora, M.Danziger, J.De Jaeger, ThomasDe Cia, A.Della Valle, M.Dennefeld, M.Elias Rosa, N.Elman, N.Feindt, U.Fleury, M.Gall, E.González Gaitán, SantiagoGalbany, LluisMorales Garoffolo, A.Greggio, L.Guillou, L. L.Hachinger, S.Hadjiyska, E.Hage, P. E.Hillebrandt, W.Hodgkin, S.Hsiao, E. Y.James, P. A.Jerkstrand, A.Kangas, T.Kankare, E.Kotak, R.Kromer, M.Kuncarayakti, H.Leloudas, G.Lundqvist, P.Lyman, J. D.Hook, I. M.Maguire, K.Manulis, I.Margheim, S.Mattila, S.Maund, J. R.Mazzali, P.McCrum, M.McKinnon, R.Moreno Raya, M. E.Nicholl, M.Nugent, P. E.Pain, R.Pignata Libralato, GiulianoPhillips, M. M.Polshaw, J.Pumo, M. L.Rabinowitz, D.Reilly, E.Romero Cañizales, C.Scalzo, R.Schmidt, B.Schulze, SteveSim, S. A.Sollerman, J.Taddia, F.Tartaglia, L.Terreran, G.Tomasella, L.Turatto, M.Walker, E.Walton, N. A.Wyrzykowski, L.Yuan, F.Zampieri, L.[PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects]

Nicholl, M.Smartt, S. J.Jerkstrand, A.Inserra, C.Sim, S. A.Chen, T. W.Benetti, S.Fraser, M.Gal Yam, AvishayKankare, E.Maguire, K.Smith, K.Sullivan, M.Valenti, S.Young, D. R.Baltay, C.Bauer, F. E.Baumont, S.Bersier, D.Botticella, M.-T.Childress, M.Dennefeld, M.Valle, M. DellaElías-Rosa, N.Feindt, U.Galbany, LluisHadjiyska, E.Le Guillou, L.Leloudas, G.Mazzali, P.McKinnon, R.Polshaw, J.Rabinowitz, D.Rostami, S.Scalzo, R.Schmidt, B. P.Schulze, SteveSollerman, J.Taddia, F.Yuan, F.[Erratum: On the diversity of superluminous supernovae: ejected mass as the dominant factor]

Gutiérrez, C.P.Anderson, J.P.Sullivan, M.Dessart, L.González-Gaitan, S.Galbany, L.Dimitriadis, G.Arcavi, I.Bufano, F.Chen, T.-W.Dennefeld, M.Gromadzki, M.Haislip, J.B.Hosseinzadeh, G.Howell, D.A.Inserra, C.Kankare, E.Leloudas, G.Maguire, K.McCully, C.Morrell, N.Olivares, E.F.Pignata, G.Reichart, D.E.Reynolds, T.Smartt, S.J.Sollerman, J.Taddia, F.Takáts, K.Terreran, G.Valenti, S.Young, D.R.[Type II supernovae in low-luminosity host galaxies]Type II supernovae in low-luminosity host galaxies

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