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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]

Barbarino, C.Dall'Ora, M.Botticella, M. T.Della Valle, MassimoZampieri, L.Maund, J.Pumo, M.Jerkstrand, A.Benetti, S.Elias Rosa, N.Fraser, M.Gal Yam, AvishayHamuy Wackenhut, MarioInserra, C.Knapic, C.LaCluyze, A.Molinaro, M.Ochner, P.Pastorello, A.Pignata Libralato, GiulianoReichart, D.Ries, C.Riffeser, A.Schmidt, B.Schmidt, M.Smareglia, R.Smartt, S.Smith, K.Sollerman, J.Sullivan, M.Tomasella, L.Turatto, M.Valenti, S.Yaron, O.Young, D.[SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phase]

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]

Hsiao, EricBurns, C. R.Contreras, C.Höflich, P.Sand, D.Marion, G. H.Phillips, M. M.Stritzinger, M.González Gaitán, FranciscoMason, R. E.Folatelli, GastónParent, E.Gall, C.Amanullah, R.Anupama, G. C.Arcavi, I.Banerjee, D. P. K.Beletsky, Y.Blanc Mendiberri, GuillermoBloom, J. S.Brown, P. J.Campillay, A.Cao, Y.De Cia, A.Diamond, T.Freedman, W. L.González, C.Goobar, A.Holmbo, S.Howell, D. A.Johansson, J.Kasliwal, M. M.Kirshner, R. P.Krisciunas, K.Kulkarni, S. R.Maguire, K.Milne, P. A.Morrell, N.Nugent, P. E.Ofek, E. O.Osip, D.Palunas, P.Perley, D. A.Persson, S. E.Piro, A. L.Rabus, M.Roth, M.Schiefelbein, J. M.Srivastav, S.Sullivan, M.Suntzeff, Nicholas B.Surace, J.Woźniak, P. R.Yaron, O.[Strong near-infrared carbon in the Type Ia supernova iPTF13ebh]

Gall, H.Polshaw, J.Kotak, R.Jerkstrand, A.Leibundgut, B.Rabinowitz, D.Sollerman, J.Sullivan, M.Smartt, S.Anderson, J.Benetti, S.Baltay, C.Feindt, U.Fraser, M.González Gaitán, SantiagoInserra, C.Maguire, K.McKinnon, R.Valenti, S.Young, D.[A comparative study of Type II-P and II-L supernova rise times as exemplified by the case of LSQ13cuw]

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