TeV gamma rays from PSR 1706-44

Details TeV gamma rays from PSR 1706-44 TeV gamma rays from PSR 1706-44

1998-04-22

arxiv.org/abs/astro-ph/9804224v1

Astropart.Phys. 9 (1998) 131-136

Astronomy and Astrophysics

Astrophysics

9 pages, 3 figures, accepted for publication in Astroparticle Physics

Scientific paper

10.1016/S0927-6505(98)00017-6

Observations made with the University of Durham Mark 6 atmospheric Cerenkov telescope confirm that PSR B1706-44 is a very high energy gamma-ray emitter. There is no indication from our dataset that the very high energy gamma-rays are pulsed, in contrast to the findings at < 20 GeV, which indicate that more than 80% of the flux is pulsed. The flux at E > 300 GeV is estimated to be (3.9 +/- 0.7 (statistical)) x 10^-11 cm^-2 s^-1.

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