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The AXAF CCD imaging spectrometerThe AXAF CCD Imaging Spectrometer (ACIS) is currently being defined as a possible focal plane instrument to be flown on the Advanced X-ray Astrophysics Facility (AXAF). The imaging spectrometer consists of an array of charge coupled devices (CCD's) to be placed at the focus of the AXAF mirrors. The array will provide high angular resolution (0.5 arc seconds), moderate spectral resolution (150 eV) over the energy range 0.1 to 10 keV, temporal resolution down to 60 microseconds, and single photon quantum detection efficiencies of up to 90 percent. X-ray sensitivity for a point source exceeds 10 to the -15th ergs/sq cm sec for a 10 to the 5th sec exposure. When used in conjunction with the objective gratings, the array will yield wavelength resolution of up to 200.
Document ID
19870032482
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Garmire, G. P.
(Pennsylvania State Univ. University Park, PA, United States)
Burrows, D.
(Pennsylvania State Univ. University Park, PA, United States)
Feigelson, E.
(Pennsylvania State Univ. University Park, PA, United States)
Nousek, J.
(Pennsylvania State University University Park, United States)
Canizares, C.
(Pennsylvania State Univ. University Park, PA, United States)
Clark, G.
(MIT Cambridge, MA, United States)
Collins, S. A.
(Pennsylvania State Univ. University Park, PA, United States)
Morrison, J.
(Pennsylvania State Univ. University Park, PA, United States)
Pravdo, S. H.
(Pennsylvania State Univ. University Park, PA, United States)
Riegler, G. R.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Subject Category
Spacecraft Instrumentation
Accession Number
87A19756
Funding Number(s)
CONTRACT_GRANT: NAG8-526
Distribution Limits
Public
Copyright
Other

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