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The Smithsonian Astrophysical Observatory (SAO) in collaboration with Stanford Research Institute (SRI) has been developing monolithic CMOS detectors for use as astronomical soft X-ray imaging spectrometers since 2008. The long term goal of this collaboration is to produce X-ray Active Pixel Sensor (APS) detectors with Fano limited performance over the 0.1-10keV band for "Facility Class" missions such as Lynx. Since CMOS x-ray imagers consume very little power; are inherently "radiation hard"; have high levels of integration ...
Published by: Proceedings of SPIE - The International Society for Optical Engineering Published on:
Cameras; CMOS integrated circuits; gamma rays; MOS devices; Neutron detectors; Particle beams; Photons; Pixels; Silicon wafers; Small satellites; Space optics; Spectrometers; X rays; Parker Engineering