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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]

Anderson, JosephJames, Phil A.Habergham, StaceyGalbany, LluisKuncarayakti, Hanindyo[Statistical Studies of Supernova Environments]

Marino, SebastiánGonzález Gaitán, SantiagoFörster, FranciscoFolatelli, GastónHamuy Wackenhut, MarioHsiao, Eric[Searching for light echoes due to circumstellar matter in SNe la Spectra]

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]

Galbany, LluisMoreno Raya, M.Ruiz Lapuente, P.González Hernández, J.Méndez, J.Vallely, P.Baron, E.Domínguez, I.Hamuy Wackenhut, MarioLópez Sánchez, Ángel R.Mollá, M.Catalán, S.Cooke, E.Fariña, C.Génova Santos, R.Karjalainen, R.Lietzen, H.McCormac, J.Riddick, F.Rubiño Martín, J.Skillen, I.Tudor, V.Vaduvescu, O.[SN 2014J at M82 – I. A middle-class Type Ia supernova by all spectroscopic metrics]

Tanaka, MasaomiTominaga, NozomuMorokuma, TomokiYasuda, NaokiFurusawa, HisanoriBaklanov, PetrBlinnikov, SergeiMoriya, TakashiDoi, MamoruJiang, Ji-AnKato, TakahiroKikuchi, YukiKuncarayakti, HanindyoNagao, TohruNomoto, Ken’ichiTaniguchi, Yuki[Rapidly Rising Transients from the Subaru Hyper Suprime-Cam Transient Survey]

Hsiao, EricBurns, C. R.Contreras, C.Höflich, P.Sand, D.Marion, G. H.Phillips, M. M.Stritzinger, M.González Gaitán, FranciscoMason, R. E.Folatelli, GastónParent, E.Gall, C.Amanullah, R.Anupama, G. C.Arcavi, I.Banerjee, D. P. K.Beletsky, Y.Blanc Mendiberri, GuillermoBloom, J. S.Brown, P. J.Campillay, A.Cao, Y.De Cia, A.Diamond, T.Freedman, W. L.González, C.Goobar, A.Holmbo, S.Howell, D. A.Johansson, J.Kasliwal, M. M.Kirshner, R. P.Krisciunas, K.Kulkarni, S. R.Maguire, K.Milne, P. A.Morrell, N.Nugent, P. E.Ofek, E. O.Osip, D.Palunas, P.Perley, D. A.Persson, S. E.Piro, A. L.Rabus, M.Roth, M.Schiefelbein, J. M.Srivastav, S.Sullivan, M.Suntzeff, Nicholas B.Surace, J.Woźniak, P. R.Yaron, O.[Strong near-infrared carbon in the Type Ia supernova iPTF13ebh]

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]

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