X-Ray Performance of a Customized Large-format Scientific CMOS Detector

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC(2022)

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摘要
In recent years, the performance of Scientific Complementary Metal Oxide Semiconductor (sCMOS) sensors has been improved significantly. Compared with charge-coupled Device sensors, sCMOS sensors have various advantages, making them potentially better devices for optical and X-ray detection, especially in time-domain astronomy. After a series of tests of sCMOS sensors, we proposed a new dedicated high-speed, large-format X-ray detector in 2016 cooperating with Gpixel Inc. This new sCMOS sensor has a physical size of 6 cm x 6 cm, with an array of 4096 x 4096 pixels and a pixel size of 15 mu m. The frame rate is 20.1 fps under current condition and can be boosted to a maximum value around 100 fps. The epitaxial thickness is increased to 10 mu m compared to the previous sCMOS product. We show the results of its first taped-out product in this work. The dark current of this sCMOS is lower than 10 e(-) pixel(-1) s(-1) at 20 degrees C, and lower than 0.02 e(-) pixel(-1) s(-1) at -30 degrees C. The fixed pattern noise and the readout noise are lower than 5 e(-) in high-gain situation and show a small increase at low temperature. The energy resolution reaches 180.1 eV (3.1%) at 5.90 keV for single-pixel events and 212.3 eV (3.6%) for all split events. The continuous X-ray spectrum measurement shows that this sensor is able to response to X-ray photons from 500 eV to 37 keV. The excellent performance, as demonstrated from these test results, makes sCMOS sensor an ideal detector for X-ray imaging and spectroscopic application.
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关键词
X-ray detectors, Astronomical instrumentation, Astronomical detectors
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