TY - JOUR
T1 - Characterization of random telegraph noise in an H2RG X-ray hybrid CMOS detector
AU - Bevidas, William A.
AU - Colosimo, Joseph M.
AU - Falcone, Abraham D.
AU - Emeigh, Timothy
AU - Stone, Lukas R.
AU - Nizam, Kadri M.
AU - Bortree, Brynn
AU - Buffington, Jacob C.
AU - Burrows, David Nelson
AU - Catlin, Zachary E.
AU - Gremling, Killian M.
AU - Hossen, Md Arman
AU - Reichard, Collin
AU - Scigliani, Ana C.
AU - Tavana, Anthony J.
AU - Wages, Mitchell
N1 - Publisher Copyright:
© The Authors.
PY - 2025/4/1
Y1 - 2025/4/1
N2 - Hybrid CMOS detectors (HCDs) have several excellent features as high-performance X-ray detectors, including rapid readout, deep-depletion silicon for high quantum efficiency, radiation hardness, and low power. Random telegraph noise (RTN) is a type of noise that can reduce the performance of HCDs and other CMOS sensors. After finding and quantifying RTN in the recently developed engineering grade Speedster-EXD550 HCDs, this form of noise has also been found in other X-ray HCDs. We aim to investigate its presence and characteristics in the relatively mature H2RG X-ray HCD and to compare it with that of the SpeedsterEXD550. We use archival data taken with an H2RG X-ray HCD at two different temperatures to determine the percentage of pixels that are being impacted by RTN. We identify RTN in 0.42% of pixels when the detector is operated at 140 K, but we are only able to identify RTN in 0.060% of pixels when the detector is operated at 160 K. We characterize RTN in two Speedster-EXD550 detectors, identifying 5.1% of pixels with RTN in one detector and 7.1% in another, which is significantly more than the H2RG. These results verify the difference between two different HCDs and provide techniques that can be applied to future HCDs.
AB - Hybrid CMOS detectors (HCDs) have several excellent features as high-performance X-ray detectors, including rapid readout, deep-depletion silicon for high quantum efficiency, radiation hardness, and low power. Random telegraph noise (RTN) is a type of noise that can reduce the performance of HCDs and other CMOS sensors. After finding and quantifying RTN in the recently developed engineering grade Speedster-EXD550 HCDs, this form of noise has also been found in other X-ray HCDs. We aim to investigate its presence and characteristics in the relatively mature H2RG X-ray HCD and to compare it with that of the SpeedsterEXD550. We use archival data taken with an H2RG X-ray HCD at two different temperatures to determine the percentage of pixels that are being impacted by RTN. We identify RTN in 0.42% of pixels when the detector is operated at 140 K, but we are only able to identify RTN in 0.060% of pixels when the detector is operated at 160 K. We characterize RTN in two Speedster-EXD550 detectors, identifying 5.1% of pixels with RTN in one detector and 7.1% in another, which is significantly more than the H2RG. These results verify the difference between two different HCDs and provide techniques that can be applied to future HCDs.
UR - https://www.scopus.com/pages/publications/105010350333
UR - https://www.scopus.com/inward/citedby.url?scp=105010350333&partnerID=8YFLogxK
U2 - 10.1117/1.JATIS.11.2.026002
DO - 10.1117/1.JATIS.11.2.026002
M3 - Article
AN - SCOPUS:105010350333
SN - 2329-4124
VL - 11
JO - Journal of Astronomical Telescopes, Instruments, and Systems
JF - Journal of Astronomical Telescopes, Instruments, and Systems
IS - 2
M1 - 026002
ER -