Very high energy gamma ray astrophysics

Details Very high energy gamma ray astrophysics Very high energy gamma ray astrophysics

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983isu..rept.....l&link_type=abstract

Technical Progress Report, Apr. 1982 - Mar. 1983 Iowa State Univ. of Science and Technology, Ames.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Cosmic Rays, Crab Nebula, Electromagnetic Radiation, Gamma Rays, Photons, Elementary Particles, Ionizing Radiation, Radiation Detectors, Supernova Remnants

Scientific paper

Sources of very high energy gamma rays (E(BETA) (11) eV) and improvement of the instrumentation of detectors in this energy regime were investigated. Approximately 4 x 10(5) Cerepkov air shower events from the region of Cygnus X-3 and the Crab nebula were collected with the JPL instrumentation during the fall of 1982. Significant improvement on the 1981 sensitivity to source variations and the development of a Cerenkov air shower camera are reported. A suitable mirror and mount for use as a detector auxiliary to the primary 10 inch Mt. Hopkins detector is located.

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