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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]

We present optical imaging and spectroscopy of supernova (SN) LSQ13fn, a type II supernova with several hitherto-unseen properties. Although it initially showed strong symmetric spectral emission features attributable to He ii, N iii, and C iii, reminiscent of some interacting SNe, it transitione...


Polshaw, J.Kotak, R.Dessart, L.Fraser, M.Gal-Yam, A.Inserra, C.Sim, S. A.Smartt, S. J.Sollerman, J.Baltay, C.Rabinowitz, D.Benetti, S.Botticella, M. T.Campbell, H.Chen, T.-W.Galbany, L.McKinnon, R.Nicholl, M.Smith, K. W.Sullivan, M.Takáts, K.Valenti, S.Young, D. R.[LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation]LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation

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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