TeV Observations of Selected GeV Sources with the HEGRA IACT-System

Details TeV Observations of Selected GeV Sources with the HEGRA IACT-System TeV Observations of Selected GeV Sources with the HEGRA IACT-System

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2329r&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

2

Scientific paper

Results from a search for TeV γ -ray emission from the vicinity of five Xray-studied GeV sources is presented. A number of possible X-ray counterparts have been suggested based on ASCA and ROSAT observations (e.g. the SNR CTA 1, and X-ray binary LS I+61° 303). Our search has yielded no convincing evidence for TeV emission at these GeV source positions and also a number possible counterparts. Preliminary upper limits in the range ˜1% to 10% of the Crab flux have been estimated above various energy thresholds 0.7 to 1.3 TeV.

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