Abstract The wealth of observational material provided by the COS-B and SAS-2 telescopes has provided a great incentive to develop new and better techniques for high energy gamma-ray astronomy. The prospects of achieving a greater sensitivity and a much improved angular resolution in future gamma-ray telescopes are reviewed in the light of the predicted performance of payloads already approved and new techniques being developed in the laboratory.
Prospects in instrumentation for future space experiments
Advances in Space Research ; 3 , 4 ; 31-38
1983-01-01
8 pages
Article (Journal)
Electronic Resource
English
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