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A balloon-borne imaging gamma-ray telescopeA balloon-borne coded-aperture gamma-ray telescope for galactic and extragalactic astronomy observations is described. The instrument, called GRIP (Gamma Ray Imaging Payload), is designed for measurements in the energy range from 30 keV to 5 MeV with an angular resolution of 0.6 deg over a 20 deg field of view. Distinguishing characteristics of the telescope are a rotating hexagonal coded-aperture mask and a thick NaI scintillation camera. Rotating hexagonal coded-apertures and the development of thick scintillation cameras are discussed.
Document ID
19850024736
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Althouse, W. E.
(California Inst. of Tech. Pasadena, CA, United States)
Cook, W. R.
(California Inst. of Tech. Pasadena, CA, United States)
Cummings, A. C.
(California Inst. of Tech. Pasadena, CA, United States)
Finger, M. H.
(California Inst. of Tech. Pasadena, CA, United States)
Prince, T. A.
(California Inst. of Tech. Pasadena, CA, United States)
Schindler, S. M.
(California Inst. of Tech. Pasadena, CA, United States)
Starr, C. H.
(California Inst. of Tech. Pasadena, CA, United States)
Stone, E. C.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Contrib. to the 19th Intern. Cosmic Ray Conf.
Subject Category
Astronomy
Report/Patent Number
OG-9.2-2
Accession Number
85N33049
Funding Number(s)
CONTRACT_GRANT: NGR-05-002-160
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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