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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]

Kankare, E.Kotak, R.Pastorello, A.Fraser, M.Mattila, S.Smartt, S.Bruce, A.Chambers, K.Elias Rosa, N.Flewelling, H.Fremling, C.Harmanen, J.Huber, M.Jerkstrand, A.Kangas, T.Kuncarayakti, HanindyoMagee, M.Magnier, E.Polshaw, J.Smith, K.Sollerman, j.Tomasella, L.[On the triple peaks of SNHunt248 in NGC 5806*]

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.Sim, S. A.Inserra, C.Anderson, J. P.Baltay, C.Benetti, S.Chambers, K.Chen, T. W.Elias Rosa, N.Feindt, U.Flewelling, H. A.Fraser, M.Gal Yam, AvishayGalbany, LluisHuber, M. E.Kangas, T.Kankare, E.Kotak, R.Kruehler, T.Maguire, K.McKinnon, R.Rabinowitz, D.Rostami, S.Schulze, SteveSmith, K.W.Sullivan, M.Tonry, J. L.Valenti, S.Young, D. R.[LSQ14bdq: A Type Ic super-luminous supernova with a double-peaked light curve]

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]

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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