H.E.S.S. unidentified sources: how can Fermi GST help?

Details H.E.S.S. unidentified sources: how can Fermi GST help? H.E.S.S. unidentified sources: how can Fermi GST help?

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1112..211t&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS: Proceedings of the 6th Edition: Bridging the Gap Between G

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Cosmic Rays, Gamma-Ray Sources, Gamma-Ray Bursts, Interactions Of Particles And Radiation With Matter

Scientific paper

H.E.S.S. is currently the most sensitive instrument in the very-high-energy (VHE >100 GeV) gamma-ray domain and has revealed many new sources along the Galactic Plane. After the very successful first VHE Galactic survey of 2004/2005, H.E.S.S. continued and extended that survey in 2006/2007, discovering a number of new sources, many of which are unidentified. Some of the unidentified H.E.S.S. sources have no counterparts at any other wavelength; some of them have X-ray counterparts, but most of them have no counterparts at GeV energies, i.e. among unidentified EGRET sources. Hence the Fermi GST observations could be a key point in order to identify them and to explain the physical processes that rule these sources.

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