Search for emission at 100 GeV from the Crab pulsar in correlation with giant pulses in radio

Details Search for emission at 100 GeV from the Crab pulsar in correlation with giant pulses in radio Search for emission at 100 GeV from the Crab pulsar in correlation with giant pulses in radio

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..apr.b8004n&link_type=abstract

American Physical Society, 2009 APS April Meeting, May 2-5, 2009, abstract #B8.004

Physics

Scientific paper

Pulsars are sources of non-thermal emission from radio energies to about 100 GeV gamma rays. In radio, some pulsars emit strong pulses, which last between a few microseconds and a few nanoseconds. The origin of these giant pulses is not understood but some argue that the emission of gamma-rays and giant pulses is tightly linked. Studies in gamma rays with the EGRET satellite did not find correlated emission with giant pulses. We present results of simultaneous radio-GeV observations with GBT and VERITAS that aim to correlate for the first time radio giant pulses with gamma rays above 100 GeV.

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