Model-based analysis of the Galactic Centre with H.E.S.S. during Summer 2003

Details Model-based analysis of the Galactic Centre with H.E.S.S. during Summer 2003 Model-based analysis of the Galactic Centre with H.E.S.S. during Summer 2003

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..397r&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

Galactic Center, Bar, Circumnuclear Matter, And Bulge, Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

The detection of a very high energy γ-ray source in the direction of the Galactic Centre with the H.E.S.S. array of Cerenkov has been reported in [1]. Another chain of analysis, including different calibration, simulation, image analysis and spectral reconstruction, has been used within the H.E.S.S. collaboration. The results of this model-based analysis are reported.

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