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Janesick, J.; Elliott, T.; Collins, S.; Daud, T.; Campbell, D.; Dingizian, A.; Garmire, G.
X-ray instrumentation in astronomy1985
X-ray instrumentation in astronomy1985
AbstractAbstract
[en] A theoretical model is presented which predicts the output response of CCD to soft X-ray spectra. The model simulates the four fundamental parameters that ultimately limit CCD performance: Quantum efficiency, charge collection efficiency, charge transfer efficiency, and read noise. Simulated results are presented for a wide variety of CCD structures, and general conclusions are presented about achieving a practical balance of sensitivity, energy, and spatial resolution for an AXAF instrument. The authors compare the results of the analysis to an existing state-of-the-art CCD and project improvements which will be made in the near future
Source
Cuhlane, J.L; p. 364-380; 1985; p. 364-380; Society of Photo-Optical Instrumentation Engineers; Bellingham, WA (USA); Conference on X-ray instrumentation in astronomy; Cannes (France); 2-4 Dec 1985
Record Type
Book
Literature Type
Conference
Country of publication
ASTRONOMY, ASTROPHYSICS, CHARGE-COUPLED DEVICES, COMPUTERIZED SIMULATION, ENERGY RESOLUTION, MATHEMATICAL MODELS, PERFORMANCE, QUANTUM EFFICIENCY, RESEARCH PROGRAMS, RESOLUTION, RESPONSE FUNCTIONS, SENSITIVITY, SIGNAL-TO-NOISE RATIO, SOFT X RADIATION, SPATIAL RESOLUTION, X-RAY DETECTION, X-RAY SPECTROMETERS, X-RAY SPECTROSCOPY
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