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A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions

In this paper, we report on the development of a monolithic active pixel sensor for X-ray imaging using 0.2 µm fully depleted silicon-on-insulator (SOI)-based technology to support next generation astronomical satellite missions. Detail regarding low-noise dual-gain SOI based pixels with a charge se...

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Detalles Bibliográficos
Autores principales: Shrestha, Sumeet, Kawahito, Shoji, Kamehama, Hiroki, Nakanishi, Syunta, Yasutomi, Keita, Kagawa, Keiichiro, Teranishi, Nobukazu, Takeda, Ayaki, Tsuru, Takeshi Go, Kurachi, Ikuo, Arai, Yasuo
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6022047/
https://www.ncbi.nlm.nih.gov/pubmed/29865217
http://dx.doi.org/10.3390/s18061789
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author Shrestha, Sumeet
Kawahito, Shoji
Kamehama, Hiroki
Nakanishi, Syunta
Yasutomi, Keita
Kagawa, Keiichiro
Teranishi, Nobukazu
Takeda, Ayaki
Tsuru, Takeshi Go
Kurachi, Ikuo
Arai, Yasuo
author_facet Shrestha, Sumeet
Kawahito, Shoji
Kamehama, Hiroki
Nakanishi, Syunta
Yasutomi, Keita
Kagawa, Keiichiro
Teranishi, Nobukazu
Takeda, Ayaki
Tsuru, Takeshi Go
Kurachi, Ikuo
Arai, Yasuo
author_sort Shrestha, Sumeet
collection PubMed
description In this paper, we report on the development of a monolithic active pixel sensor for X-ray imaging using 0.2 µm fully depleted silicon-on-insulator (SOI)-based technology to support next generation astronomical satellite missions. Detail regarding low-noise dual-gain SOI based pixels with a charge sensitive amplifier and pinned depleted diode sensor structure is presented. The proposed multi-well sensor structure underneath the fully-depleted SOI allows the design of a detector with low node capacitance and high charge collection efficiency. Configurations for achieving very high charge-to-voltage conversion gain of 52 µV/e(−) and 187 µV/e(−) are demonstrated. Furthermore, in-pixel dual gain selection is used for low-noise and wide dynamic range X-ray energy detection. A technique to improve the noise performance by removing correlated system noise leads to an improvement in the spectroscopic performance of the measured X-ray energy. Taken together, the implemented chip has low dark current (44.8 pA/cm(2) at −30 °C), improved noise performance (8.5 e(−) rms for high gain and 11.7 e(−) rms for low gain), and better energy resolution of 2.89% (171 eV FWHM) at 5.9 keV using (55)Fe and 1.67% (234 eV FWHM) at 13.95 keV using (241)Am.
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spelling pubmed-60220472018-07-02 A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions Shrestha, Sumeet Kawahito, Shoji Kamehama, Hiroki Nakanishi, Syunta Yasutomi, Keita Kagawa, Keiichiro Teranishi, Nobukazu Takeda, Ayaki Tsuru, Takeshi Go Kurachi, Ikuo Arai, Yasuo Sensors (Basel) Article In this paper, we report on the development of a monolithic active pixel sensor for X-ray imaging using 0.2 µm fully depleted silicon-on-insulator (SOI)-based technology to support next generation astronomical satellite missions. Detail regarding low-noise dual-gain SOI based pixels with a charge sensitive amplifier and pinned depleted diode sensor structure is presented. The proposed multi-well sensor structure underneath the fully-depleted SOI allows the design of a detector with low node capacitance and high charge collection efficiency. Configurations for achieving very high charge-to-voltage conversion gain of 52 µV/e(−) and 187 µV/e(−) are demonstrated. Furthermore, in-pixel dual gain selection is used for low-noise and wide dynamic range X-ray energy detection. A technique to improve the noise performance by removing correlated system noise leads to an improvement in the spectroscopic performance of the measured X-ray energy. Taken together, the implemented chip has low dark current (44.8 pA/cm(2) at −30 °C), improved noise performance (8.5 e(−) rms for high gain and 11.7 e(−) rms for low gain), and better energy resolution of 2.89% (171 eV FWHM) at 5.9 keV using (55)Fe and 1.67% (234 eV FWHM) at 13.95 keV using (241)Am. MDPI 2018-06-01 /pmc/articles/PMC6022047/ /pubmed/29865217 http://dx.doi.org/10.3390/s18061789 Text en © 2018 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
spellingShingle Article
Shrestha, Sumeet
Kawahito, Shoji
Kamehama, Hiroki
Nakanishi, Syunta
Yasutomi, Keita
Kagawa, Keiichiro
Teranishi, Nobukazu
Takeda, Ayaki
Tsuru, Takeshi Go
Kurachi, Ikuo
Arai, Yasuo
A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title_full A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title_fullStr A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title_full_unstemmed A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title_short A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions
title_sort silicon-on-insulator-based dual-gain charge-sensitive pixel detector for low-noise x-ray imaging for future astronomical satellite missions
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6022047/
https://www.ncbi.nlm.nih.gov/pubmed/29865217
http://dx.doi.org/10.3390/s18061789
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