Paper
19 October 1993 Soft gamma-ray telescope for space flight use
Upendra D. Desai, Jay P. Norris, R. J. Nemiroff
Author Affiliations +
Abstract
Soft (gamma) -ray imaging instruments onboard currently operating astrophysical observatories attain angular resolutions on the order of 10 arc minutes using coded apertures with uniformly redundant arrays. In crowded regions, e.g. the galactic plane and center regions, unambiguous association with candidates at other wavelengths will often require improved localizations. We discuss a (gamma) -ray telescope design using 'chirp-Z' function codes and coarse position-sensitive image plane detectors. Image plane detector systems consisting of CsI scintillators and avalanche photodiodes are evaluated. Position sensitivity is achieved by either using a matrix of individual CsI/APD detectors or CsI scintillator rods. The aim is to design a narrow field-of-view telescope with sub-arcminute resolution to be flown on a small spacecraft.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Upendra D. Desai, Jay P. Norris, and R. J. Nemiroff "Soft gamma-ray telescope for space flight use", Proc. SPIE 1948, Astroparticle Physics and Novel Gamma-Ray Telescopes, (19 October 1993); https://doi.org/10.1117/12.161376
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Cited by 4 scholarly publications.
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KEYWORDS
Space telescopes

Telescopes

Gamma radiation

Sensors

Image sensors

Scintillators

Coded aperture imaging

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