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

Bruno Khélifi (1) , Nukri Komin (2) , Thomas Lohse (2) , Conor Masterson (2) , Stefan Schlenker (2) , Fabian Schmidt (2) , U. Schwanke (2) , Christian Stegmann (2)

1 MPIK - Max-Planck-Institut für Kernphysik
2 Institut für Physik

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

Mots clés: ENERGY GAMMA-RAYS; CRAB; SYSTEM; JET

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⟩