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  1. 原著論文

Proton radiation hardness of x-ray SOI pixel sensors with pinned depleted diode structure

https://repo.qst.go.jp/records/85274
https://repo.qst.go.jp/records/85274
41dbb4e5-b9c0-4b7f-a66b-3c480d7d1599
Item type 学術雑誌論文 / Journal Article(1)
公開日 2021-12-28
タイトル
タイトル Proton radiation hardness of x-ray SOI pixel sensors with pinned depleted diode structure
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 Mitsuki, Hayashida

× Mitsuki, Hayashida

WEKO 1027976

Mitsuki, Hayashida

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Hagino, Kouichi

× Hagino, Kouichi

WEKO 1027977

Hagino, Kouichi

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Kohmura, Takayoshi

× Kohmura, Takayoshi

WEKO 1027978

Kohmura, Takayoshi

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Masatoshi, Kitajima

× Masatoshi, Kitajima

WEKO 1027979

Masatoshi, Kitajima

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Yarita, Keigo

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WEKO 1027980

Yarita, Keigo

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Oono, Kenji

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WEKO 1027981

Oono, Kenji

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Negishi, Kousuke

× Negishi, Kousuke

WEKO 1027982

Negishi, Kousuke

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G. Tsuru, Takeshi

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WEKO 1027983

G. Tsuru, Takeshi

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Tanaka, Takaaki

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WEKO 1027984

Tanaka, Takaaki

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Hiroyuki, Uchida

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WEKO 1027985

Hiroyuki, Uchida

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Kayama, Kazuho

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WEKO 1027986

Kayama, Kazuho

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Kodama, Ryota

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WEKO 1027987

Kodama, Ryota

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Koji, Mori

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WEKO 1027988

Koji, Mori

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Ayaki, Takeda

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WEKO 1027989

Ayaki, Takeda

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Yusuke, Nishioka

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WEKO 1027990

Yusuke, Nishioka

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Hida, Takahiro

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WEKO 1027991

Hida, Takahiro

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Yukumoto, Masataka

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WEKO 1027992

Yukumoto, Masataka

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Arai, Yasuo

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WEKO 1027993

Arai, Yasuo

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Kurachi, Ikuo

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WEKO 1027994

Kurachi, Ikuo

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Hisashi, Kitamura

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WEKO 1027995

Hisashi, Kitamura

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Kawahito, Shoji

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WEKO 1027996

Kawahito, Shoji

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Yasutomi, Keita

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WEKO 1027997

Yasutomi, Keita

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Mitsuki, Hayashida

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WEKO 1027998

en Mitsuki, Hayashida

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Masatoshi, Kitajima

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WEKO 1027999

en Masatoshi, Kitajima

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Yarita, Keigo

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WEKO 1028000

en Yarita, Keigo

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Oono, Kenji

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WEKO 1028001

en Oono, Kenji

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Negishi, Kousuke

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WEKO 1028002

en Negishi, Kousuke

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Hiroyuki, Uchida

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WEKO 1028003

en Hiroyuki, Uchida

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Koji, Mori

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WEKO 1028004

en Koji, Mori

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Ayaki, Takeda

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WEKO 1028005

en Ayaki, Takeda

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Yusuke, Nishioka

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WEKO 1028006

en Yusuke, Nishioka

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Hisashi, Kitamura

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WEKO 1028007

en Hisashi, Kitamura

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抄録
内容記述タイプ Abstract
内容記述 X-ray silicon-on-insulator (SOI) pixel sensors, “XRPIX,” are being developed for the next-generation x-ray astronomical satellite, “FORCE.” The XRPIX is fabricated with the SOI technology, which makes it possible to integrate a high-resistivity Si sensor and a low-resistivity Si complementary metal oxide semiconductor (CMOS) circuit. The CMOS circuit in each pixel is equipped with a trigger function, allowing us to read out outputs only from the pixels with x-ray signals at the timing of x-ray detection. This function thus realizes high throughput and high time resolution, which enables to employ anti-coincidence technique for background rejection. A new series of XRPIX named XRPIX6E developed with a pinned depleted diode (PDD) structure improves spectral performance by suppressing the interference between the sensor and circuit layers. When semiconductor x-ray sensors are used in space, their spectral performance is generally degraded owing to the radiation damage caused by high-energy protons. Therefore, before using an XRPIX in space, it is necessary to evaluate the extent of degradation of its spectral performance by radiation damage. Thus, we performed a proton irradiation experiment for XRPIX6E for the first time at Heavy Ion Medical Accelerator in Chiba in the National Institute of Radiological Sciences. We irradiated XRPIX6E with high-energy protons with a total dose of up to 40 krad, equivalent to 400 years of irradiation in orbit. The 40-krad irradiation degraded the energy resolution of XRPIX6E by 25  ±  3  %  , yielding an energy resolution of 260.1  ±  5.6  eV at the full-width half maximum for 5.9 keV X-rays. However, the value satisfies the requirement for FORCE, 300 eV at 6 keV, even after the irradiation. It was also found that the PDD XRPIX has enhanced radiation hardness compared to previous XRPIX devices. In addition, we investigated the degradation of the energy resolution; it was shown that the degradation would be due to increasing energy-independent components, e.g., readout noise.
書誌情報 Journal of Astronomical Telescopes, Instruments, and Systems

巻 7, p. 036001, 発行日 2021-08
ISSN
収録物識別子タイプ ISSN
収録物識別子 2329-4124
DOI
識別子タイプ DOI
関連識別子 10.1117/1.JATIS.7.3.036001
関連サイト
識別子タイプ DOI
関連識別子 https://doi.org/10.1117/1.JATIS.7.3.036001
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