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Search for TeV Emission from the Direction of the Vela and PSR B1706-44 Pulsars with the H.E.S.S. Experiment
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Search for TeV Emission from the Direction of the Vela and PSR B1706-44 Pulsars with the H.E.S.S. Experiment

Bruno Khélifi, Nukri Komin, Thomas Lohse, Conor Masterson, Stefan Schlenker, Fabian Schmidt, U. Schwanke, Christian Stegmann et HESS collaboration
High Energy Gamma-Ray Astronomy, AIP CONFERENCE PROCEEDINGS, Vol.745(1), pp.335-340
2nd International Symposium on High Energy Gamma-Ray Astronomy
01/01/2005
DOI: https://doi.org/10.1063/1.1878426

Résumé

SYSTEM JET ENERGY GAMMA-RAYS CRAB
The pulsar wind nebulae (PWN) around the Vela and PSR B1706-44 pulsars have been observed in 2003 and 2004 with the H.E.S.S. Cherenkov telescopes. No evidence of a g-ray emission from either source is seen and upper limits on the integrated flux are reported

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