Pulsed emission of very high energy gamma rays from Crab Pulsar.

Details Pulsed emission of very high energy gamma rays from Crab Pulsar. Pulsed emission of very high energy gamma rays from Crab Pulsar.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acpsn...8...63x&link_type=abstract

Acta Phys. Sin., Overseas Ed., Vol. 8, No. 1, p. 63 - 70

Physics

Pulsars: Gamma Rays

Scientific paper

The authors present here the results of observation of very high energy (VHE) gamma-ray emission from Crab Pulsar with the Beijing Atmospheric Cerenkov Telescopes, named ACT2 and ACT3, during the 1995 - 1996 season. The data are based on 168 hr (ACT2) and 125 hr (ACT3) of exposure over the period of observation in tracking mode. After converting the event time to the solar barycentre, the data have been searched for evidence of pulsed emission at the 33 ms period of the Crab Pulsar. The authors found no steady emission of VHE gamma-rays with a 33 ms period on the time scale of months or nights. But there are two pieces of evidence of sporadic emission of over an hour duration with the same period as the one in the radio wave band.

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