A gamma-ray telescope for the 1980's

Details A gamma-ray telescope for the 1980's A gamma-ray telescope for the 1980's

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jbis...35..290c&link_type=abstract

British Interplanetary Society, Journal (Space Technology), vol. 35, July 1982, p. 290-296.

Mathematics

Logic

Angular Resolution, Gamma Ray Telescopes, High Resolution, Technological Forecasting, Energy Spectra, Gamma Ray Astronomy, Gamma Ray Spectra, Photosensitivity, Systems Simulation

Scientific paper

The methods by which low energy gamma-ray astronomical telescopes progress from the basic collimated instrument, with an angular resolution of a few deg, to a sophisticated two-dimensional imaging instrument capable of identifying gamma-ray sources at other wavelengths are described. A low energy gamma-ray telescope with arcmin resolution in the 0.1-10 MeV range, which employs a novel method of obtaining position resolution in inorganic scintillators while retaining high shielding efficiency and good energy resolution, is discussed with a view to both its design features and simulated observational capabilities.

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