Abstract
The EGRET experiment detected pulsed emission from several pulsars in the HE energy range 20 MeV 130 GeV and detecting the signature periodicity of pulsars if it exists. Data recorded on the Crab pulsar with the Whipple Imaging Atmospheric Cerenkov Telescope has been analysed with this software and upper limits on pulsed emission have been obtained.
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Schedule a callMore From: Proceedings of the International Astronomical Union. International Astronomical Union
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