论文信息 - Development of the Buckland Park Cosmic Ray Air Shower Array for Ultra High Energy Gamma Ray Astronomy

Development of the Buckland Park Cosmic Ray Air Shower Array for Ultra High Energy Gamma Ray Astronomy

Abstract The Buckland Park air shower array is being developed particularly for use as an ultra-high-energy gamma ray astronomy telescope. The properties of this instrument are described with an emphasis on improvements being made to its angular resolution. Some early data are presented to illustrate the way in which the data obtained will be used.

P. Edwards | D. Ciampa | J. Patterson | R. Clay | C. L. Corani

[1] R. Clay,et al. Fast timing of air shower fronts , 1986 .

[2] R. Clay,et al. First observation of ultra-high-energy γ rays from LMC X-4 , 1985, Nature.

[3] R. Clay,et al. First observation of gamma-rays from VELA X-1 at energies greater than 3 X 10 to the 15th eV , 1984 .

[4] R. Clay,et al. Design and performance of the buckland park air shower array , 1981 .