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 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998hepnp..22....4x&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 22, No. 1, p. 4 - 12

Physics

Pulsars: Gamma Rays

Scientific paper

Presents the results of observation of very high energy (VHE) gamma-ray emission from the Crab Pulsar with Beijing Atmospheric Čerenkov Telescopes, named ACT2 and ACT3, for the duration of the boreal fall 1995 - spring 1996 season. The data are based on 168 hours (ACT2) and 125 hours (ACT3) of exposure over the period of observation in tracking mode. After conversion of the event time to the solar barycenter, 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 33-ms period at the month or night scales. However, there were two examples of sporadic emission over an hour in duration with the same period as the radio frequency emission.

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