VHE gamma rays from PSR B1706-44

Details VHE gamma rays from PSR B1706-44 VHE gamma rays from PSR B1706-44

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..612c&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 612-616 (1997).

Computer Science

1

Pulsars, Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

Observations made with the University of Durham Mark 6 atmospheric Čerenkov telescope confirm that PSR B1706-44 is a VHE γ-ray emitter. The γ-ray flux has been measured at 250 GeV, and suggests a spectral slope that is consistent with extrapolation from the sub-10 GeV region. There is no indication from our dataset that the VHE γ-rays are pulsed, in contrast to the findings at <20 GeV, which indicate that 100% of the flux is pulsed.

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