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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.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]

Maguire, K.Sullivan, M.Patat, F.Gal-Yam, A.Hook, I. M.Dhawan, S.Howell, D. A.Mazzali, P.Nugent, P. E.Pan, Y. C.Podsiadlowski, P.Simon, J. D.Sternberg, A.Valenti, S.Baltay, C.Bersier, D.Blagorodnova, N.Chen, T. W.Ellman, N.Feindt, U.Förster, FranciscoFraser, M.González Gaitán, SantiagoGraham, M. L.Gutiérrez, C.Hachinger, S.Hadjiyska, E.Inserra, C.Knapic, C.Laher, R. R.Leloudas, G.Margheim, S.McKinnon, R.Molinaro, M.Morrell, N.Ofek, E. O.Rabinowitz, D.Rest, A.Sand, D.Smareglia, R.Smartt, S. J.Taddia, F.Walker, E. S.Walton, N. A.Young, D. R.[A statistical analysis of circumstellar material in Type Ia supernovae]

Kangas, T.Mattila, S.Kankare, E.Lundqvist, P.Vaeisaenen, P.Childress, M.Pignata Libralato, GiulianoMcCully, C.Valenti, S.Vinkó, J.Pastorello, A.Elias Rosa, N.Fraser, M.Gal Yam, AvishayKotak, R.Kotilainen, J. K.Smartt, S. J.Galbany, LluisHarmanen, J.Howell, D. A.Inserra, C.Marion, G. H.Quimby, R. M.Silverman, J. M.Szalai, T.Wheeler, J. C.Ashall, C.Benetti, S.Romero Cañizales, C.Smith, K. W.Sullivan, M.Takáts, K.Young, D. R.[Supernova 2013fc in a circumnuclear ring of a luminous infrared galaxy: the big brother of SN 1998S]

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