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000644454 005__ 20260125055220.0
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000644454 0247_ $$2arXiv$$aarXiv:2512.16005
000644454 0247_ $$2datacite_doi$$a10.3204/PUBDB-2026-00331
000644454 037__ $$aPUBDB-2026-00331
000644454 041__ $$aEnglish
000644454 088__ $$2arXiv$$aarXiv:2512.16005
000644454 1001_ $$aBrun, Francois$$b0
000644454 245__ $$aHEGS : Revisiting a decade of H.E.S.S. extragalactic observations
000644454 260__ $$c2025
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000644454 500__ $$aPresented at the 39th International Cosmic Ray Conference (ICRC 2025)
000644454 520__ $$aDuring its first phase, from 2004 up to the end of 2012, the H.E.S.S. (High Energy StereoscopicSystem) experiment observed the extragalactic skies for more than 2700 hours. These data have been re-analysed in a single consistent framework, leading to the derivation of a catalog of 23 sources. In total, about 5.7% of the sky was observed, allowing for several additional studies to be conducted: source variability, extragalactic gamma-ray background light, and comparison with the Fermi-LAT catalogues. In this contribution, we discuss these results and present the high-level data (catalogs, maps) released to the astrophysical community.
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000644454 7001_ $$aSanchez, David$$b1
000644454 7001_ $$0P:(DE-H253)PIP1080492$$aTaylor, Andrew$$b2$$eCorresponding author$$udesy
000644454 7001_ $$aCerruti, Matteo$$b3
000644454 7001_ $$aLenain, Jean-Philippe$$b4
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