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Article
The Oriented Scintillation Spectrometer Experiment - Instrument Description
The Astrophysical Journal
  • J. D. Kurfess, Naval Research Lab
  • W. N. Johnson, Naval Research Lab
  • R. L. Kinzer, Naval Research Lab
  • R. A. Kroeger, Naval Research Lab
  • M. S. Stickman, Naval Research Lab
  • J. E. Grove, Naval Research Lab
  • Mark D Leising, Clemson University
  • D. D. Clayton, Clemson University
  • D. A. Grabelsky, Northwestern University
  • W. R. Purcell, Northwestern University
Document Type
Article
Publication Date
8-27-1992
Publisher
IOP Publishing
Abstract

The Oriented Scintillation Spectrometer Experiment on the Arthur Holly Compton Gamma Ray Observatory satellite uses four actively shielded NaI (Tl)-CsI(Na) phoswich detectors to provide gamma-ray line and continuum detection capability in the 0.05-10 MeV energy range. The instrument includes secondary capabilities for gamma-ray and neutron detection between 10 and 250 MeV. The detectors have 3.8 deg x 11.04 deg (FWHM) fields of view defined by tungsten collimators. Each detector has an independent, single-axis orientation system which permits offset pointing from the spacecraft Z-axis for background measurements and multitarget observations. The instrument, and its calibration and performance, are described.

Comments

Additional authors: R.A. Kroeger, M.S. Strickman, J.E. Grove, D.A. Grabelsky, W.R. Purcell, M.P. Ulmer, R.A. Cameron, G.V. Jung

Citation Information
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