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

doi:https://doi.org/10.1063/1.1878426

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

B. Khélifi-2005-01-01-AIP conference proceedings

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TL;DRAbstract

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 γ‐ray emission from either source is seen and upper limits on the integrated flux are reported.

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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 γ‐ray emission from either source is seen and upper limits on the integrated flux are reported.

Keywords

VelaPulsarPhysicsCherenkov radiationAstrophysicsAstronomyFlux (metallurgy)Optics

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