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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]

Scalzo, R. A.Aldering, G.Antilogus, P.Aragón, C.Bailey, S.Baltay, C.Bongard, S.Buton, C.Childress, M.Chotard, N.Copin, Y.Fakhouri, H. K.Gal Yam, AvishayGangler, E.Hoyer, SergioKasliwal, M.Loken, S.Nugent, P.Pain, R.Pécontal, E.Pereira, R.Perlmutter, S.Rabinowitz, DavidRau, A.Rigaudier, G.Runge, K.Smadja, G.Tao, C.Thomas, R. C.Weaver, B.Wu, C.[NEARBY SUPERNOVA FACTORY OBSERVATIONS OF SN 2007IF: FIRST TOTAL MASS MEASUREMENT OF A SUPER-CHANDRASEKHAR-MASS PROGENITOR]

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]

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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