Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM

Kazuki Yoshida; Daisuke Yonetoku; Tatsuya Sawano; Hirokazu Ikeda; Atsushi Harayama; Makoto Arimoto; Yasuaki Kagawa; Masao Ina; Satoshi Hatori; Kyo Kume; Satoshi Mizushima; Takashi Hasegawa

doi:10.1117/12.2231370

Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM

Kazuki Yoshida, Daisuke Yonetoku, Tatsuya Sawano, Hirokazu Ikeda, Atsushi Harayama, Makoto Arimoto, Yasuaki Kagawa, Masao Ina, Satoshi Hatori, Kyo Kume, Satoshi Mizushima, Takashi Hasegawa

Waseda Research Institute for Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

4 Citations (Scopus)

Abstract

We are planning a future gamma-ray burst (GRB) mission HiZ-GUNDAM to probe the early universe beyond the redshift of z > 7. Now we are developing a small prototype model of wide-field low-energy X-ray imaging detectors to observe high-z GRBs, which cover the energy range of 1 - 20 keV. In this paper, we report overview of its prototype system and performance, especially focusing on the characteristics and radiation tolerance of high gain analog ASIC specifically designed to read out small charge signals.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Publisher	SPIE
Volume	9905
ISBN (Electronic)	9781510601895
DOIs	https://doi.org/10.1117/12.2231370
Publication status	Published - 2016
Event	Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray - Edinburgh, United Kingdom Duration: 2016 Jun 26 → 2016 Jul 1

Other

Other	Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Country/Territory	United Kingdom
City	Edinburgh
Period	16/6/26 → 16/7/1

Keywords

ASIC
gamma-ray burst
radiation hardness
satellite
single event upset
X-ray

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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10.1117/12.2231370

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Yoshida, K, Yonetoku, D, Sawano, T, Ikeda, H, Harayama, A, Arimoto, M, Kagawa, Y, Ina, M, Hatori, S, Kume, K, Mizushima, S & Hasegawa, T 2016, Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM. in Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. vol. 9905, 99050M, SPIE, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, Edinburgh, United Kingdom, 16/6/26. https://doi.org/10.1117/12.2231370

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abstract = "We are planning a future gamma-ray burst (GRB) mission HiZ-GUNDAM to probe the early universe beyond the redshift of z > 7. Now we are developing a small prototype model of wide-field low-energy X-ray imaging detectors to observe high-z GRBs, which cover the energy range of 1 - 20 keV. In this paper, we report overview of its prototype system and performance, especially focusing on the characteristics and radiation tolerance of high gain analog ASIC specifically designed to read out small charge signals.",

keywords = "ASIC, gamma-ray burst, radiation hardness, satellite, single event upset, X-ray",

author = "Kazuki Yoshida and Daisuke Yonetoku and Tatsuya Sawano and Hirokazu Ikeda and Atsushi Harayama and Makoto Arimoto and Yasuaki Kagawa and Masao Ina and Satoshi Hatori and Kyo Kume and Satoshi Mizushima and Takashi Hasegawa",

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doi = "10.1117/12.2231370",

language = "English",

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note = "Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray ; Conference date: 26-06-2016 Through 01-07-2016",

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T1 - Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM

AU - Yoshida, Kazuki

AU - Yonetoku, Daisuke

AU - Sawano, Tatsuya

AU - Ikeda, Hirokazu

AU - Harayama, Atsushi

AU - Arimoto, Makoto

AU - Kagawa, Yasuaki

AU - Ina, Masao

AU - Hatori, Satoshi

AU - Kume, Kyo

AU - Mizushima, Satoshi

AU - Hasegawa, Takashi

PY - 2016

Y1 - 2016

N2 - We are planning a future gamma-ray burst (GRB) mission HiZ-GUNDAM to probe the early universe beyond the redshift of z > 7. Now we are developing a small prototype model of wide-field low-energy X-ray imaging detectors to observe high-z GRBs, which cover the energy range of 1 - 20 keV. In this paper, we report overview of its prototype system and performance, especially focusing on the characteristics and radiation tolerance of high gain analog ASIC specifically designed to read out small charge signals.

AB - We are planning a future gamma-ray burst (GRB) mission HiZ-GUNDAM to probe the early universe beyond the redshift of z > 7. Now we are developing a small prototype model of wide-field low-energy X-ray imaging detectors to observe high-z GRBs, which cover the energy range of 1 - 20 keV. In this paper, we report overview of its prototype system and performance, especially focusing on the characteristics and radiation tolerance of high gain analog ASIC specifically designed to read out small charge signals.

KW - ASIC

KW - gamma-ray burst

KW - radiation hardness

KW - satellite

KW - single event upset

KW - X-ray

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DO - 10.1117/12.2231370

M3 - Conference contribution

AN - SCOPUS:85003703936

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BT - Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray

PB - SPIE

T2 - Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray

Y2 - 26 June 2016 through 1 July 2016

ER -

Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM

Abstract

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Keywords

ASJC Scopus subject areas

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