Discovery of VHE and HE emission from the blazar 1ES 0414+009 with H.E.S.S and Fermi-LAT

F. Volpe; L. Costamante; L. G\'erard (the HESS collaboration); M. Ajello (the Fermi-LAT Collaboration); M. Hauser; S. Fegan; S. Kaufmann; S. Ohm

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Discovery of VHE and HE emission from the blazar 1ES 0414+009 with H.E.S.S and Fermi-LAT

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arxiv 1105.5114 v1 pith:VY7SD6WL submitted 2011-05-25 astro-ph.HE

F. Volpe , S. Ohm , M. Hauser , S. Kaufmann , L. Gérard (the HESS collaboration) , L. Costamante , S. Fegan , M. Ajello (the Fermi-LAT Collaboration) This is my paper · ORCID

classification astro-ph.HE

keywords energyhighdetectedaboveabsorptionareabackgroundblazar

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The high energy peaked BL Lac (HBL) object 1ES 0414+009 (z=0.287) is a distant very high-energy (VHE, E > 100 GeV) blazars with well-determined redshift. This source was detected with the High Energy Stereoscopic System (H.E.S.S.) between October 2005 and September 2009. It was also detected with the Fermi Large Area Telescope (LAT) in 21 months of data. The combined high energy (HE) and VHE spectra, once corrected for gamma-gamma absorption on the extragalactic background light (EBL), indicate a Compton peak located above few TeV, among the highest in the BL Lac class.

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