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- W1549920413 abstract "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." @default.
- W1549920413 created "2016-06-24" @default.
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- W1549920413 date "2009-01-01" @default.
- W1549920413 modified "2023-09-27" @default.
- W1549920413 title "H.E.S.S. unidentified sources: how can Fermi GST help?" @default.
- W1549920413 doi "https://doi.org/10.1063/1.3125784" @default.
- W1549920413 hasPublicationYear "2009" @default.
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