Details

Autor(en) / Beteiligte

• Anderhub, H
• Antonelli, L. A
• Backes, M
• Barrio, J. A
• Bastieri, D
• Berger, al K
• Bock, R. K
• Bordas, P
• Tridon, D. Borla
• Bosch-Ramon, V
• Bose, D
• Bretz, T
• Britzger, D
• Camara, M
• Colin, P
• Commichau, S
• Contreras, J. L
• Costado, M. T
• Covino, S
• De Angelis, A
• de Cea del Pozo, E
• De Sabata, F
• Dorner, D
• Doro, M
• Elsaesser, D
• Errando, M
• Ferenc, D
• Font, L
• Galante, N
• Garczarczyk, M
• Goebel, F
• Herrero, A
• Hildebrand, D
• Höhne-Mönch, D
• Hose, J
• Hrupec, D
• Hsu, C. C
• Jogler, T
• Klepser, S
• Barbera, A. La
• Laille, A
• Leonardo, E
• Lindfors, E
• Lombardi, S
• Longo, F
• Lorenz, E
• Majumdar, P
• Mannheim, K
• Maraschi, L
• Mariotti, M
• Martínez, M
• Meucci, M
• Miranda, J. M
• Mirzoyan, R
• Miyamoto, H
• Moles, M
• Moralejo, A
• Nieto, D
• Nilsson, K
• Ninkovic, J
• Paoletti, R
• Paredes, J. M
• Pasanen, M
• Pascoli, D
• Pauss, F
• Pegna, R. G
• Perez-Torres, M. A
• Persic, M
• Peruzzo, L
• Prada, F
• Prandini, E
• Puljak, I
• Reichardt, I
• Rhode, W
• Ribó, M
• Rissi, M
• Rügamer, S
• Saggion, A
• Saito, T. Y
• Sánchez-Conde, M
• Satalecka, K
• Scalzotto, V
• Schweizer, T
• Shore, S. N
• Sierpowska-Bartosik, A
• Sillanpää, A
• Sitarek, J
• Sobczynska, D
• Spiro, S
• Stamerra, A
• Stark, L. S
• Takalo, L
• Tavecchio, F
• Torres, D. F
• Wagner, R. M
• Zabalza, V
• Zandanel, F
• Zanin, R
• Zapatero, J
• Cognard, I

Titel

Search for Very High Energy Gamma-ray Emission from Pulsar-Pulsar Wind Nebula Systems with the MAGIC Telescope

Ist Teil von

• The Astrophysical journal, 2010-02, Vol.710 (1), p.828-835

Ort / Verlag

Bristol: IOP Publishing

Erscheinungsjahr

2010

Link zum Volltext

Quelle

EZB Electronic Journals Library

Beschreibungen/Notizen

• The MAGIC collaboration has searched for high-energy gamma-ray emission of some of the most promising pulsar candidates above an energy threshold of 50 GeV, an energy not reachable up to now by other ground-based instruments. Neither pulsed nor steady gamma-ray emission has been observed at energies of 100 GeV from the classical radio pulsars PSR J0205+6449 and PSR J2229+6114 (and their nebulae 3C58 and Boomerang, respectively) and the millisecond pulsar PSR J0218+4232. Here, we present the flux upper limits for these sources and discuss their implications in the context of current model predictions.