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24 August 2021 Radiation testing of a back illuminated, small pixel, CMOS compatible CCD
Beverly J. LaMarr, Marshall Bautz, Barry Burke, Michael Cooper, Kevan Donlon, Richard Foster, Catherine E. Grant, Andrew Malonis, Eric Miller, Gregory Prigozhin
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Proceedings Volume 11821, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII; 118211G (2021) https://doi.org/10.1117/12.2594797
Event: SPIE Optical Engineering + Applications, 2021, San Diego, California, United States
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Abstract
Next-generation X-ray imaging missions require fast, low-noise detectors that can survive the harsh environment of space without significant loss of performance. As part of a detector development effort toward a mission such as Lynx, we report on the effects of proton exposure on the spectral performance, dark current and charge transfer efficiency of a back illuminated MIT Lincoln Laboratory CCID93. The CCD has 8 micron pixels and can be clocked with 2.5MHz pixel speeds with CMOS compatible voltage swings. The 40 MeV proton dose is chosen to represent typical on orbit exposure. Variations with charge injection, temperature, and clocking speed are explored. These results are compared with those of the front illuminated version of the same device.
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Beverly J. LaMarr, Marshall Bautz, Barry Burke, Michael Cooper, Kevan Donlon, Richard Foster, Catherine E. Grant, Andrew Malonis, Eric Miller, and Gregory Prigozhin "Radiation testing of a back illuminated, small pixel, CMOS compatible CCD", Proc. SPIE 11821, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII, 118211G (24 August 2021); https://doi.org/10.1117/12.2594797
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KEYWORDS
Sensors
Back illuminated sensors
Charge-coupled devices
X-rays
Detector development
Spectral resolution
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