TeV gamma rays from PSR 1706-44
/ Authors
P. Chadwick, M. Dickinson, N. Dipper, J. Holder, T. Kendall, T. Mccomb, K. Orford, J. Osborne, S. Rayner, I. Roberts
and 2 more authors
/ Abstract
Observations made with the University of Durham Mark 6 atmospheric Cerenkov telescope conrm that PSR B1706-44 is a very high energy -ray emitter. There is no indication from our dataset that the very high energy -rays are pulsed, in contrast to the ndings at 300 GeV is estimated to be (3:90:7stat)10 11 cm 2 s 1 .
Journal: Astroparticle Physics