Paper
9 September 2019 Event-driven detectors for soft x-ray astronomy
Author Affiliations +
Abstract
We discuss the joint development by Penn State University (PSU) and Teledyne Imaging Systems (TIS) of hybrid CMOS detectors for X-ray astronomy, and specifically the development over the past 10 years of a new event-driven X-ray detector for future astronomy missions. This novel X-ray detector is designed to perform onchip event recognition and to read out only pixels containing X-ray events. With the exception of analog power supply voltages, the detector is digital in/digital out, reducing off-chip electronics to a minimum. It operates at frame rates of over 1000 frames per second, providing excellent performance for bright X-ray sources and/or high-throughput optics. The pixel size is 40 × 40 microns, and we are fabricating devices with 550 × 550 pixels.
© (2019) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David N. Burrows, Abraham D. Falcone, Jianmei Pan, Vincent Douence, and Yibin Bai "Event-driven detectors for soft x-ray astronomy", Proc. SPIE 11118, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXI, 1111803 (9 September 2019); https://doi.org/10.1117/12.2528530
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KEYWORDS
Sensors

X-ray astronomy

CMOS sensors

Readout integrated circuits

X-ray detectors

Analog electronics

Detector development

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