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