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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]

Stritzinger, M.Valenti, S.Hoeflich, P.Baron, E.Phillips, M.Taddia, F.Foley, R.Hsiao, EricJha, S.McCully, C.Pandya, V.Simon, J.Benetti, S.Brown, P.Burns, C.Campillay, A.Contreras, C.Förster Burón, FranciscoHolmbo, S.Marion, G.Morrell, N.Pignata Libralato, Giuliano[Comprehensive observations of the bright and energetic Type lax SN 2012Z: Interpretation as a Chandrasekhar mass white dwarf explosion]

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]

Gall, C.Stritzinger, M.D.Ashall, C.Baron, E.Burns, C.R.Hoeflich, P.Hsiao, E.Y.Mazzali, P.A.Phillips, M.M.Filippenko, A.V.Anderson, J.P.Benetti, S.Brown, P.J.Campillay, A.Challis, P.Contreras, C.Elias De La Rosa, N.Folatelli, G.Foley, R.J.Fraser, M.Holmbo, S.Marion, G.H.Morrell, N.Pan, Y.-C.Pignata, G.Suntzeff, N.B.Taddia, F.Robledo, S.T.Valenti, S.[Two transitional type Ia supernovae located in the Fornax cluster member NGC 1404: SN 2007on and SN 2011iv]Two transitional type Ia supernovae located in the Fornax cluster member NGC 1404: SN 2007on and SN 2011iv

SNhunt151 was initially classified as a supernova (SN) impostor (nonterminal outburst of a massive star). It exhibited a slow increase in luminosity, lasting about 450 d, followed by a major brightening that reaches M V ≈ -18 mag. No source is detected to M V ≳ -13 mag in archival images at the p...


Elias-Rosa, N.Benetti, S.Cappellaro, E.Pastorello, A.Terreran, G.Morales-Garoffolo, A.Howerton, S.C.Valenti, S.Kankare, E.Drake, A.J.Djorgovski, S.G.Tomasella, L.Tartaglia, L.Kangas, T.Ochner, P.Filippenko, A.V.Ciabattari, F.Geier, S.Howell, D.A.Isern, J.Leonini, S.Pignata, G.Turatto, M.[SNhunt151: An explosive event inside a dense cocoon]SNhunt151: An explosive event inside a dense cocoon

Tomasella, L.Cappellaro, E.Pumo, M.L.Jerkstrand, A.Benetti, S.Elias-Rosa, N.Fraser, M.Inserra, C.Pastorello, A.Turatto, M.Anderson, J.P.Galbany, L.Gutiérrez, C.P.Kankare, E.Pignata, G.Terreran, G.Valenti, S.Barbarino, C.Bauer, F.E.Botticella, M.T.Chen, T.-W.Gal-Yam, A.Harutyunyan, A.Howell, D.A.Maguire, K.Garoffolo, A.M.Ochner, P.Smartt, S.J.Schulze, S.Young, D.R.Zampieri, L.[SNe 2013K and 2013am: Observed and physical properties of two slow, normal Type IIP events]SNe 2013K and 2013am: Observed and physical properties of two slow, normal Type IIP events

Barbarino, C.Dall'Ora, M.Botticella, M. T.Della Valle, MassimoZampieri, L.Maund, J.Pumo, M.Jerkstrand, A.Benetti, S.Elias Rosa, N.Fraser, M.Gal Yam, AvishayHamuy Wackenhut, MarioInserra, C.Knapic, C.LaCluyze, A.Molinaro, M.Ochner, P.Pastorello, A.Pignata Libralato, GiulianoReichart, D.Ries, C.Riffeser, A.Schmidt, B.Schmidt, M.Smareglia, R.Smartt, S.Smith, K.Sollerman, J.Sullivan, M.Tomasella, L.Turatto, M.Valenti, S.Yaron, O.Young, D.[SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phase]

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

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