The AXAF CCD imaging spectrometerThe current status of the instrument design and the status of the CCDs being fabricated for the AXAF CCD Imaging Spectrometer (ACIS) are summarized. The instrument consists of an image recording array of CCDs and a linear arrangement of CCDs to record the spectra formed by the objective grating spectrometer. Both arrays employ CCDs with pixel dimensions which correspond to about 0.5 arcsec samples of the image. The CCDs provide moderate spectral resolution and good detection efficiency over the energy range 0.5 to 10 keV. Spectral resolution of 200 or more is achievable using the objective grating with the grating array. Radiation damage effects are shown to degrade the energy resolution of CCDs. Specially designed CCD pixel architecture is employed together with shielding and low temperature operation to slow the effects of radiation damage.
Document ID
19920055968
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Garmire, G. P. (Pennsylvania State University University Park, United States)
Ricker, G. R. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Bautz, M. W. (MIT Cambridge, MA, United States)
Burke, B. (MIT Lexington, MA, United States)
Burrows, D. N. (Pennsylvania State University University Park, United States)
Collins, S. A. (JPL Pasadena, CA, United States)
Doty, J. P. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Gendreau, K. (MIT Cambridge, MA, United States)
Lumb, D. H. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Nousek, J. A. (Pennsylvania State University University Park, United States)
Date Acquired
August 15, 2013
Publication Date
March 1, 1992
Subject Category
Astronomy
Report/Patent Number
AIAA PAPER 92-1473Report Number: AIAA PAPER 92-1473