Very high energy gamma-ray observation of the peculiar transient event Swift J1644+57 with the MAGIC telescopes and AGILE




Aleksic J, Antonelli LA, Antoranz P, Asensio M, Backes M, de Almeida UB, Barrio JA, Gonzalez JB, Bednarek W, Berger K, Bernardini E, Biland A, Blanch O, Bock RK, Boller A, Bonnefoy S, Bonnoli G, Tridon DB, Bretz T, Carmona E, Carosi A, Fidalgo DC, Colin P, Colombo E, Contreras JL, Cortina J, Cossio L, Covino S, Da Vela P, Dazzi F, De Angelis A, De Caneva G, De Lotto B, Mendez CD, Doert M, Dominguez A, Prester DD, Dorner D, Doro M, Eisenacher D, Elsaesser D, Farina E, Ferenc D, Fonseca MV, Font L, Fruck C, Lopez RJG, Garczarczyk M, Terrats DG, Gaug M, Giavitto G, Godinovic N, Munoz AG, Gozzini SR, Hadamek A, Hadasch D, Herrero A, Hose J, Hrupec D, Idec W, Jankowski F, Kadenius V, Klepser S, Knoetig ML, Krahenbuhl T, Krause J, Kushida J, La Barbera A, Lelas D, Lewandowska N, Lindfors E, Lombardi S, Lopez M, Lopez-Coto R, Lopez-Oramas A, Lorenz E, Lozano I, Makariev M, Mallot K, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Marcote B, Mariotti M, Martinez M, Masbou J, Mazin D, Meucci M, Miranda JM, Mirzoyan R, Moldon J, Moralejo A, Munar-Adrover P, Nakajima D, Niedzwiecki A, Nilsson K, Nowak N, Orito R, Paiano S, Palatiello M, Paneque D, Paoletti R, Paredes JM, Partini S, Persic M, Prada F, Moroni PGP, Prandini E, Puljak I, Reichardt I, Reinthal R, Rhode W, Ribo M, Rico J, Saggion A, Saito K, Saito TY, Salvati M, Satalecka K, Scalzotto V, Scapin V, Schultz C, Schweizer T, Shore SN, Sillanpaa A, Sitarek J, Snidaric I, Sobczynska D, Spanier F, Spiro S, Stamatescu V, Stamerra A, Steinke B, Storz J, Sun S, Suric T, Takalo L, Takami H, Tavecchio F, Temnikov P, Terzic T, Tescaro D, Teshima M, Tibolla O, Torres DF, Toyama T, Treves A, Uellenbeck M, Vogler P, Wagner RM, Weitzel Q, Zandanel F, Zanin R, Longo F, Lucarelli F, Pittori C, Verrecchia F

PublisherEDP SCIENCES S A

2013

Astronomy and Astrophysics

ASTRONOMY & ASTROPHYSICS

ASTRON ASTROPHYS

ARTN A112

552

6

0004-6361

DOIhttps://doi.org/10.1051/0004-6361/201321197

http://www.aanda.org/articles/aa/pdf/2013/04/aa21197-13.pdf



Results. No clear evidence for emission above the energy threshold of 100 GeV was found. MAGIC observations permit one to constrain the emission from the source down to 100 GeV, which favors models that explain the observed lower energy variable emission. Data analysis of simultaneous observations from AGILE, Fermi and VERITAS also provide negative detection, which additionally constrain the self-Compton emission component.



Last updated on 2024-26-11 at 22:40