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Astrophysics > Instrumentation and Methods for Astrophysics

arXiv:2310.14887 (astro-ph)
[Submitted on 23 Oct 2023 (v1), last revised 4 Dec 2023 (this version, v2)]

Title:An Aluminum-coated sCMOS sensor for X-Ray Astronomy

Authors:Qinyu Wu, Zhixing Ling, Chen Zhang, Shuang-Nan Zhang, Weimin Yuan
View a PDF of the paper titled An Aluminum-coated sCMOS sensor for X-Ray Astronomy, by Qinyu Wu and 4 other authors
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Abstract:In recent years, tremendous progress has been made on scientific Complementary Metal Oxide Semiconductor (sCMOS) sensors, making them a promising device for future space X-ray missions. We have customized a large-format sCMOS sensor, G1516BI, dedicated for X-ray applications. In this work, a 200 nm thick aluminum layer is successfully sputtered on the surface of this sensor. This Al-coated sensor, named EP4K, shows consistent performance with the uncoated version. The readout noise of the EP4K sensor is around 2.5 e- and the dark current is less than 0.01 e-/pixel/s at -30 degree. The maximum frame rate is 20 Hz in the current design. The ratio of single pixel events of the sensor is 45.0%. The energy resolution can reach 153.2 eV at 4.51 keV and 174.2 eV at 5.90 keV at -30 degree. The optical transmittance of the aluminum layer is approximately 1e-8 to 1e-10 for optical lights from 365 to 880 nm, corresponding to an effective aluminum thickness of around 140 to 160 nm. The good X-ray performance and low optical transmittance of this Al-coated sCMOS sensor make it a good choice for space X-ray missions. The Lobster Eye Imager for Astronomy (LEIA), which has been working in orbit for about one year, is equipped with four pieces of EP4K sensors. Furthermore, 48 pieces of EP4K sensors are used on the Wide-field X-ray Telescope (WXT) on the Einstein Probe (EP) satellite, which will be launched at the end of 2023.
Comments: published on PASP
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); High Energy Physics - Experiment (hep-ex); Instrumentation and Detectors (physics.ins-det)
Cite as: arXiv:2310.14887 [astro-ph.IM]
  (or arXiv:2310.14887v2 [astro-ph.IM] for this version)
  https://doi.org/10.48550/arXiv.2310.14887
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1088/1538-3873/ad03d7
DOI(s) linking to related resources

Submission history

From: Zhixing Ling Dr [view email]
[v1] Mon, 23 Oct 2023 12:55:38 UTC (2,978 KB)
[v2] Mon, 4 Dec 2023 13:31:22 UTC (2,978 KB)
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