Paper
31 October 1996 High-efficiency detector array concept for x-ray astronomy based on CCDs
Christian M. Castelli, Mark R. Sims, Alan A. Wells
Author Affiliations +
Abstract
The detection efficiency of charge coupled devices (CCDs) in the x-ray band is dependent on the thickness of the active depletion layer in the silicon. This is typically under 35 micrometer and limited by the purity of available epitaxial substrates. For x-ray imaging, this results in a reduced CCD detection efficiency above 8 keV. In this paper, we show that by using a novel illumination geometry, CCDs can detect high energy (up to 100 keV) x rays with reasonable efficiency and good energy resolution. A novel 2-D imaging had x-ray detector based on this geometry is discussed.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christian M. Castelli, Mark R. Sims, and Alan A. Wells "High-efficiency detector array concept for x-ray astronomy based on CCDs", Proc. SPIE 2808, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VII, (31 October 1996); https://doi.org/10.1117/12.256039
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KEYWORDS
Charge-coupled devices

X-rays

Sensors

Silicon

X-ray astronomy

X-ray detectors

CCD image sensors

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