EXOSS - A hard X-ray and soft gamma-ray astronomy missionThe Energetic X-ray Observatory on Space Station (EXOSS) is a mission concept for high-sensitivity coded-aperture sky surveys and studies of the spectral and temporal behavior of astrophysical sources from approximately 3 keV to 1 MeV. The scientific motivation for the mission and the instrument requirements, including the need for high angular resolution to resolve and identify numerous detectable sources, are summarized. Two baseline telescopes are described: one employing a 1.4-sq-m array of Xe gas imaging proportional counters to cover the 3 to 100 keV range with 1 arcmin resolution; the second using a 2.8-sq-m array of NaI/CsI imaging phoswich detectors to span the 20 keV to MeV range with 12 arcmin resolution.
Document ID
19920037646
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cook, W. R. (California Inst. of Tech. Pasadena, CA, United States)
Prince, T. A. (California Institute of Technology Pasadena, United States)
Grindlay, J. E. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Weisskopf, M. C. (California Inst. of Tech. Pasadena, CA, United States)
Ramsey, B. D. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Skinner, G. K. (Birmingham, University United Kingdom)
Date Acquired
August 15, 2013
Publication Date
January 1, 1990
Subject Category
Astronomy
Meeting Information
Meeting: EUV, X-ray and Gamma-Ray Instrumentation for Astronomy