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Volumn 325, Issue 5939, 2009, Pages 444-468

Radio imaging of the very-high-energy γ-ray emission region in the central engine of a radio galaxy

(388)  Acciari, V A a   Aliu, E b   Arlen, T c   Bautista, M d   Beilicke, M e   Benbow, W a   Bradbury, S M f   Buckley, J H e   Bugaev, V e   Butt, Y a   Byrum, K g   Cannon, A h   Celik, O c   Cesarini, A i   Chow, Y C c   Ciupik, L j   Cogan, P d   Cui, W k   Dickherber, R e   Fegan, S J c   more..


Author keywords

[No Author keywords available]

Indexed keywords

ACCRETION; ELECTRON; EXTRATERRESTRIAL MATTER; GAMMA RAY RADIATION; IMAGING METHOD; PLASMA;

EID: 67749112002     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1175406     Document Type: Article
Times cited : (274)

References (33)
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    • H.E.S.S, We thank the Namibian authorities and the University of Namibia for support in facilitating the construction and operation of H.E.S.S. We also thank the German Ministry for Education and Research (BMBF, the Max Planck Society, the French Ministry for Research, CNRS-IN2P3 and the Astroparticle Interdisciplinary Programme of CNRS, the U.K. Science and Technology Facilities Council STFC, the Institute of Particle and Nuclear Physics of the Charles University, the Polish Ministry of Science and Higher Education, and the South African Department of Science and Technology and National Research Foundation for support. We appreciate the excellent work of the technical support staff in Berlin, Durham, Hamburg, Heidelberg, Palaiseau, Paris, and Saclay and also in Namibia in the construction and operation of the equipment. MAGIC: We thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma, as
    • H.E.S.S.: We thank the Namibian authorities and the University of Namibia for support in facilitating the construction and operation of H.E.S.S. We also thank the German Ministry for Education and Research (BMBF), the Max Planck Society, the French Ministry for Research, CNRS-IN2P3 and the Astroparticle Interdisciplinary Programme of CNRS, the U.K. Science and Technology Facilities Council (STFC), the Institute of Particle and Nuclear Physics of the Charles University, the Polish Ministry of Science and Higher Education, and the South African Department of Science and Technology and National Research Foundation for support. We appreciate the excellent work of the technical support staff in Berlin, Durham, Hamburg, Heidelberg, Palaiseau, Paris, and Saclay and also in Namibia in the construction and operation of the equipment. MAGIC: We thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma, as well as the German BMBF and MPG, the Italian INFN and Spanish Ministerio de Ciencia e Innovación. This work was also supported by ETH research grant TH 34/043, the Polish MniSzW grant N N203 390834, and the Young Investigators Program of the Helmholtz Gemeinschaft. VERITAS: This research is supported by grants from the U.S. Department of Energy, NSF, the Smithsonian Institution, the Natural Sciences and Engineering Research Council of Canada, Science Foundation Ireland, and the STFC in the U.K. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and the collaborating institutions in the construction and operation of the instrument. VLBA: The Very Long Baseline Array is operated by the National Radio Astronomy Observatory, a facility of NSF, operated under cooperative-agreement by Associated Universities, Inc.


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