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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]

Spiro, S.Yoshii, Y.Pastorello, A.Pumo, M. L.Zampieri, L.Turatto, M.Smartt, S. J.Benetti, S.Cappellaro, E.Valenti, S.Agnoletto, I.Altavilla, G.Aoki, T.Brocato, E.Corsini, E. M.Di Cianno, A.Eliás Rosa, N.Hamuy Wackenhut, MarioEnya, K.Fiaschi, M.Folatelli, GastónDesidera, S.Harutyunyan, A.Howell, D. A.Kawka, AKobayashi, Y.Leibundgut, B.Minezaki, T.Navasardyan, H.Nomoto, K.Mattila, S.Pietrinferni, A.Pignata Libralato, GiulianoRaimondo, G.Salvo, M.Schmidt, B. P.Sollerman, J.Spyromilio, J.Taubenberger, S.Valentini, G.Vennes, S.[Low luminosity Type II supernovae – II. Pointing towards moderate mass precursors]

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

We present the complete set of ultra-violet, optical and near-infrared photometry and spectroscopy for SN 2012ca, covering the period from 6 d prior to maximum light, until 531 d after maximum. The spectroscopic time series for SN 2012ca is essentially unchanged over 1.5 yr, and appear to be domi...


Inserra, C.Fraser, M.Smartt, S. J.Benetti, S.Chen, T.-W.Childress, M.Gal-Yam, A.Howell, D. A.Kangas, T.Pignata, G.Polshaw, J.Sullivan, M.Smith, K. W.Valenti, S.Young, D. R.Parker, S.Seccull, T.McCrum, M.[On Type IIn/Ia-CSM supernovae as exemplified by SN 2012ca]On Type IIn/Ia-CSM supernovae as exemplified by SN 2012ca

Kangas, T.Mattila, S.Kankare, E.Lundqvist, P.Väisänen, P.Childress, M.Pignata, G.McCully, C.Valenti, S.Vinkó, J.Pastorello, A.Elias-Rosa, N.Fraser, M.Gal-Yam, A.Kotak, R.Kotilainen, J. K.Smartt, S. J.Galbany, L.Harmanen, 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]Supernova 2013fc in a circumnuclear ring of a luminous infrared galaxy: The big brother of SN 1998S

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