The energy spectra of TeV sources measured with the Durham Mark 6 Telescope
Chadwick, P. M. · Lyons, K. · McComb, T. J. L. · Orford, K. J. · Osborne, J. L. · Rayner, S. M. · Shaw, S. E. · Turver, K. E.
Original · EN
A programme of detailed simulations of the response of the Durham Mark 6 atmospheric Cherenkov telescope is in progress. The effective collecting area for triggering by gamma-ray showers after application of selection criteria is derived as a function of energy. An initial result from the larger events in the 1996 and 1997 observations of the BL Lac PKS 2155-304 is that the time averaged flux above 1.5 TeV was (6.7 +/- 2.2) x 10-8 m-2 s-1.
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