0000000000356714

AUTHOR

Italy 8 Istituto Nazionale Di Fisica Nucleare

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Observation of TeV gamma-rays from the unidentified source HESS J1841-055 with the ARGO-YBJ experiment

2013

We report the observation of a very high energy \gamma-ray source, whose position is coincident with HESS J1841-055. This source has been observed for 4.5 years by the ARGO-YBJ experiment from November 2007 to July 2012. Its emission is detected with a statistical significance of 5.3 standard deviations. Parameterizing the source shape with a two-dimensional Gaussian function we estimate an extension \sigma=(0.40(+0.32,-0.22}) degree, consistent with the HESS measurement. The observed energy spectrum is dN/dE =(9.0-+1.6) x 10^{-13}(E/5 TeV)^{-2.32-+0.23} photons cm^{-2} s^{-1} TeV^{-1}, in the energy range 0.9-50 TeV. The integral \gamma-ray flux above 1 TeV is 1.3-+0.4 Crab units, which is…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)PhotonDegree (graph theory)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleGamma rayFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesgamma raysWavelengthSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceCoincident0103 physical sciencesGamma Rays Argo-YBJ Extended Air Shower DetectorsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsgeneral [gamma rays]Energy (signal processing)
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