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Characteristics of the telescope for high energy gamma-ray astronomy selected for definition studies on the Gamma Ray ObservatoryThe high energy gamma-ray telescope selected for definition studies on the Gamma Ray Observatory provides a substantial improvement in observational capability over earlier instruments. It will have about 20 times more sensitivity, cover a much broader energy range, have considerably better energy resolution and provide a significantly improved angular resolution. The design and performance are described.
Document ID
19800043493
Document Type
Reprint (Version printed in journal)
Authors
Hughes, E. B. (Stanford Univ. CA, United States)
Hofstadter, R. (Stanford Univ. CA, United States)
Rolfe, J. (Stanford University Stanford, Calif., United States)
Johansson, A. (Stanford University Stanford, Calif.; Tandem Accelerator Laboratory, Uppsala, Sweden)
Bertsch, D. L. (Stanford Univ. CA, United States)
Cruickshank, W. J. (Stanford Univ. CA, United States)
Ehrmann, C. H. (Stanford Univ. CA, United States)
Fichtel, C. E. (Stanford Univ. CA, United States)
Hartman, R. C. (Stanford Univ. CA, United States)
Kniffen, D. A. (NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1980
Subject Category
Astronomy
Accession Number
80A27663
Funding Number(s)
CONTRACT_GRANT: NAS5-25544
CONTRACT_GRANT: NGR-05-020-452
Distribution Limits
Public
Copyright
Other

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