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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

Abstract : 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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https://hal-insu.archives-ouvertes.fr/insu-00356271
Contributor : Béatrice Pibaret-Bourdon Connect in order to contact the contributor
Submitted on : Tuesday, January 27, 2009 - 10:18:40 AM
Last modification on : Monday, June 15, 2020 - 12:00:33 PM

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Bruno Khélifi, Nukri Komin, Thomas Lohse, Conor Masterson, Stefan Schlenker, et al.. Search for TeV Emission from the Direction of the Vela and PSR B1706-44 Pulsars with the H.E.S.S. Experiment. 2nd International Symposium on High Energy Gamma-Ray Astronomy, 2004, Heidelberg, Germany. pp.335-340, ⟨10.1063/1.1878426⟩. ⟨insu-00356271⟩

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