MAGIC observations of very high energy gamma-rays from HESS J1813-178



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Antoranz Canales, Pedro and Barrio Uña, Juan Abel and Contreras González, José Luis and Fonseca González, Mª Victoria and López Moya, Marcos and Miranda Pantoja, José Miguel (2006) MAGIC observations of very high energy gamma-rays from HESS J1813-178. Astrophysical journal, 637 (1 (Par). L41-L44. ISSN 0004-637X

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Recently, the HESS collaboration has reported the detection of gamma-ray emission above a few hundred GeV from eight new sources located close to the Galactic plane. The source HESS J1813-178 has sparked particular interest, as subsequent radio observations imply an association with supernova remnant G12.82-0.02. Triggered by the detection in very high energy gamma-rays, a positionally coincident source has also been found in INTEGRAL and ASCA data. In this Letter we present MAGIC observations of HESS J1813-178, resulting in the detection of a differential gamma-ray flux consistent with a hard-slope power law, described as dN(gamma)/(dA dt dE) = (3.3 +/- 0.5) x 10(-12)(E/TeV)(-2.1 +/- 0.2) cm(-2) s(-1) TeV-1. We briefly discuss the observational technique used and the procedure implemented for the data analysis, and we put this detection in the perspective of multifrequency observations.

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© The American Astronomical Society. We would like to thank the IAC for the excellent working conditions at the Observatory de los Muchachos in La Palma. The support of the German BMBF and MPG, the Italian INFN, and the Spanish CICYT is gratefully acknowledged. This work was also supported by ETH research grant TH 34/04 3 and the Polish MNiI grant 1P03D01028.

Uncontrolled Keywords:Finite-Element-Method, Direct RF Exposure, Electric-Field, Biological Implications, Fluid Membranes, Mobile Phone, Vesicles, Cells, Radiation, Orientation.
Subjects:Sciences > Physics > Electronics
Sciences > Physics > Astrophysics
Sciences > Physics > Electricity
Sciences > Physics > Nuclear physics
ID Code:24353
Deposited On:24 Jan 2014 11:10
Last Modified:10 Dec 2018 14:58

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