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Aliu, E; Anderhub, H; Antoranz, P; Armada, A; Barrio, J. A; Bartko, H; Bednarek, W; Berger, K; Bigongiari, C; Biland, A; Bock, R. K; Bordas, P; Bosch-Ramon, V; Bretz, T; Camara, M; Carmona, E; Chilingarian, A; Coarasa, J. A; Commichau, S; Cortina, J; Curtef, V; Danielyan, V; Dazzi, F; De Angelis, A; Domingo-Santamaría, E; Doro, M; Errando, M; Ferenc, D; Fernández, E; Firpo, R; Flix, J; Fonseca, M. V; Font, L; Fuchs, M; Galante, N; García-López, R. J; Garczarczyk, M; Goebel, F; Hakobyan, D; Hayashida, M; Herrero, A; Höhne, D; Hose, J; Hsu, C. C; Jacon, P; Jogler, T; Kosyra, R; Kranich, D; Kritzer, R; Laille, A; Lindfors, E; Lombardi, S; López, J; López, M; Maneva, G; Mannheim, K; Mariotti, M; Martínez, M; Mazin, D; Meucci, M; Meyer, M; Miranda, J. M; Mirzoyan, R; Mizobuchi, S; Moralejo, A; Nieto, D; Oña-Wilhelmi, E; Oya, I; Paneque, D; Panniello, M; Paredes, J. M; Pasanen, M; Pascoli, D; Pauss, F; Pegna, R; Peruzzo, L; Piccioli, A; Prandini, E; Rhode, W; Ribó, M; Rico, J; Robert, A; Saggion, A; Saito, T; Sánchez, A; Sartori, P; Scalzotto, V; Schmitt, R; Schweizer, T; Shayduk, M; Shore, S. N; Sidro, N; Sillanpää, A; Stamerra, A; Temnikov, P; Torres, D. F; Turini, N; Vankov, H; Zandanel, F; Zapatero, J
The Astrophysical journal, 08/2007, Letnik: 664, Številka: 2Journal Article
We report the detection of a new source of very high energy (VHE; unk greater than or equal to 100 Gev) Y-ray emission located close to the Galactic plane, MA J0616+225, which is spatially coincident with supernova remnant IC 443. The observations were carried out with the MAGIC telescope unk 2005 December-2006 January and 2006 December-2007 January. Here we present results from this source, leading to a VHE Y-ray unk statistical significance of 5.7 sigma in the 2006/2007 data and a measured differential Y-ray flux consistent with a power law, described as unk(dAdtdE) = (1.0 plus or minus 0.2) x 10 super(11)(E/0.4TeV)-3.1 plus or minus 0.3 cm super(-2) s super(-1) Tev super(-1). we briefly discuss the observational technique used and the unk implemented for the data analysis. The results are placed in the context of the multiwavelength emission and the molecular environment region of IC 443.
