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Brocato, E.Branchesi, M.Cappellaro, E.Covino, S.Grado, A.Greco, G.Limatola, L.Stratta, G.Yang, S.Campana, S.D'Avanzo, P.Getman, F.Melandri, A.Nicastro, L.Palazzi, E.Pian, E.Piranomonte, S.Pulone, L.Rossi, A.Tomasella, L.Amati, L.Antonelli, L.A.Ascenzi, S.Benetti, S.Bulgarelli, A.Capaccioli, M.Cella, G.Dadina, M.De Cesare, G.D'Elia, V.Ghirlanda, G.Ghisellini, G.Giuffrida, G.Iannicola, G.Israel, G.Lisi, M.Longo, F.Mapelli, M.Marinoni, S.Marrese, P.Masetti, N.Patricelli, B.Possenti, A.Radovich, M.Razzano, M.Salvaterra, R.Schipani, P.Spera, M.Stamerra, A.Stella, L.Tagliaferri, G.Testa, V.[GRAWITA: VLT Survey Telescope observations of the gravitational wave sources GW150914 and GW151226]GRAWITA: VLT Survey Telescope observations of the gravitational wave sources GW150914 and GW151226

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

We present the VST Optical Imaging of the CDFS and ES1 Fields (VOICE) Survey, a VST INAF Guaranteed Time program designed to provide optical coverage of two 4 deg2 cosmic windows in the Southern hemisphere. VOICE provides the first, multi-band deep optical imaging of these sky regions, thus compl...


Vaccari, M.Covone, G.Radovich, M.Grado, A.Limatola, L.Botticella, M.T.Cappellaro, E.Paolillo, M.Pignata, G.De Cicco, D.Falocco, S.Marchetti, L.Brescia, M.S., CavuotiLongo, G.Capaccioli, M.Napolitano, N.Schipani, P.[The VOICE Survey : VST Optical Imaging of the CDFS and ES1 Fields]The VOICE Survey : VST Optical Imaging of the CDFS and ES1 Fields

Kuncarayakti, H.Maeda, K.Ashall, C.J.Prentice, S.J.Mattila, S.Kankare, E.Fransson, C.Lundqvist, P.Pastorello, A.Leloudas, G.Anderson, J.P.Benetti, S.Bersten, M.C.Cappellaro, E.Cartier, R.Denneau, L.Della Valle, M.Elias-Rosa, N.Folatelli, G.Fraser, M.Galbany, L.Gall, C.Gal-Yam, A.Gutiérrez, C.P.Hamanowicz, A.Heinze, A.Inserra, C.Kangas, T.Mazzali, P.Melandri, A.Pignata, G.Rest, A.Reynolds, T.Roy, R.Smartt, S.J.Smith, K.W.Sollerman, J.Somero, A.Stalder, B.Stritzinger, M.Taddia, F.Tomasella, L.Tonry, J.Weiland, H.Young, D.R.[SN 2017dio: A Type-Ic Supernova Exploding in a Hydrogen-rich Circumstellar Medium]SN 2017dio: A Type-Ic Supernova Exploding in a Hydrogen-rich Circumstellar Medium

It is well known that massive stars (M > 8 M ) evolve up to the collapse of the stellar core, resulting in most cases in a supernova (SN) explosion. Their heterogeneity is related mainly to different configurations of the progenitor star at the moment of the explosion and to their immediate envir...


Elias-Rosa, N.Van Dyk, S.D.Benetti, S.Cappellaro, E.Smith, N.Kotak, R.Turatto, M.Filippenko, A.V.Pignata, G.Fox, O.D.Galbany, L.González-Gaitán, S.Miluzio, M.Monard, L.A.G.Ergon, M.[The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst]The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst

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