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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]

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]

Matheson, ThomasGarnavich, P. M.Stanek, k. z.Bersier, D.Holland, S. T.Krisciunas, K.Caldwell, N.Berlind, P.Bloom, J. S.Bolte, M.Bonanos, A. Z.Brown, M. J. I.Brown, W. R.Calkins, M. L.Challis, P.Chornock, R.Echevarria, L.Eisenstein, D. J.Everett, M. E.Filippenko, A. V.Flint, K.Foley, R. J.Freedman, D. .L.Hamuy Wackenhut, MarioHarding, P.Hathi, N. P.Hicken, M.Hoopes, C.Impey, C.Jannuzi, B. T.Jansen, R. A.Jha, S.Kaluzny, J.Kannappan, S.Kirshner, R. P.Latham, D. W.Lee, J. C.Leonard, D. .C.Li, W.Luhman, K. L.Martini, P.Mathis, H.Maza Sancho, JoséMegeath, S. T.Miller, L. R.Minniti, D.Olszewski, E. W.Papenkova, M.Phillips, M. M.Pindor, B.Sasselov, D. D.Schild, R.Schweiker, H.Spahr, T.Thomas-Osip, J.Thompson, I.Weisz, D.Windhorst, R.Zaritsky, D.[PHOTOMETRY AND SPECTROSCOPY OF GRB 030329 AND ITS ASSOCIATED SUPERNOVA 2003dh: THE FIRST TWO MONTHS]

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