Achievements of the ASTRO-E hard X-ray detector development

M. Tashiro; K. Makishima; T. Kamae; T. Murakami; T. Takahashi; Y. Fukazawa; M. Kokubun; K. Nakazawa; M. Nomachi; A. Yoshida; Y. Ezoe; N. Isobe; N. Iyomoto; J. Kataoka; J. Kotoku; M. Kouda; S. Kubo; A. Kubota; Y. Matsumoto; T. Mizuno; Y. Okada; N. Ota; H. Ozawa; G. Sato; M. Sugiho; M. Sugizaki; I. Takahashi; H. Takahashi; T. Tamura; C. Tanihata; Y. Terada; Y. Uchiyama; S. Watanabe; K. Yamaoka; D. Yonetoku

Achievements of the ASTRO-E hard X-ray detector development

M. Tashiro
, K. Makishima
, T. Kamae
, T. Murakami
, T. Takahashi
, Y. Fukazawa
, M. Kokubun
, K. Nakazawa
, M. Nomachi
, A. Yoshida
, Y. Ezoe
, N. Isobe
, N. Iyomoto
, J. Kataoka
, J. Kotoku
, M. Kouda
, S. Kubo
, A. Kubota
, Y. Matsumoto
, T. Mizuno

Y. Okada, N. Ota, H. Ozawa, G. Sato, M. Sugiho, M. Sugizaki, I. Takahashi, H. Takahashi, T. Tamura, C. Tanihata, Y. Terada, Y. Uchiyama, S. Watanabe, K. Yamaoka, D. Yonetoku

Saitama University

Research output: Contribution to conference › Paper › peer-review

Abstract

The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10^-5 counts s^-1cm^-2keV^-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.

Original language	English
Pages	483-486
Number of pages	4
State	Published - 2001
Externally published	Yes
Event	2001 IEEE Nuclear Science Symposium Conference Record - San Diege, CA, United States Duration: 4 Nov 2001 → 10 Nov 2001

Conference

Conference	2001 IEEE Nuclear Science Symposium Conference Record
Country/Territory	United States
City	San Diege, CA
Period	4/11/01 → 10/11/01

Keywords

ASTRO-E
Hard X-ray detector
Sensitivity
Spectral response

Cite this

Tashiro, M., Makishima, K., Kamae, T., Murakami, T., Takahashi, T., Fukazawa, Y., Kokubun, M., Nakazawa, K., Nomachi, M., Yoshida, A., Ezoe, Y., Isobe, N., Iyomoto, N., Kataoka, J., Kotoku, J., Kouda, M., Kubo, S., Kubota, A., Matsumoto, Y., ... Yonetoku, D. (2001). Achievements of the ASTRO-E hard X-ray detector development. 483-486. Paper presented at 2001 IEEE Nuclear Science Symposium Conference Record, San Diege, CA, United States.

@conference{bb51bb758af34f768bf6ec91135dcc8e,

title = "Achievements of the ASTRO-E hard X-ray detector development",

abstract = "The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10-5 counts s-1cm-2keV-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.",

keywords = "ASTRO-E, Hard X-ray detector, Sensitivity, Spectral response",

author = "M. Tashiro and K. Makishima and T. Kamae and T. Murakami and T. Takahashi and Y. Fukazawa and M. Kokubun and K. Nakazawa and M. Nomachi and A. Yoshida and Y. Ezoe and N. Isobe and N. Iyomoto and J. Kataoka and J. Kotoku and M. Kouda and S. Kubo and A. Kubota and Y. Matsumoto and T. Mizuno and Y. Okada and N. Ota and H. Ozawa and G. Sato and M. Sugiho and M. Sugizaki and I. Takahashi and H. Takahashi and T. Tamura and C. Tanihata and Y. Terada and Y. Uchiyama and S. Watanabe and K. Yamaoka and D. Yonetoku",

year = "2001",

language = "英語",

pages = "483--486",

note = "2001 IEEE Nuclear Science Symposium Conference Record ; Conference date: 04-11-2001 Through 10-11-2001",

}

Tashiro, M, Makishima, K, Kamae, T, Murakami, T, Takahashi, T, Fukazawa, Y, Kokubun, M, Nakazawa, K, Nomachi, M, Yoshida, A, Ezoe, Y, Isobe, N, Iyomoto, N, Kataoka, J, Kotoku, J, Kouda, M, Kubo, S, Kubota, A, Matsumoto, Y, Mizuno, T, Okada, Y, Ota, N, Ozawa, H, Sato, G, Sugiho, M, Sugizaki, M, Takahashi, I, Takahashi, H, Tamura, T, Tanihata, C, Terada, Y, Uchiyama, Y, Watanabe, S, Yamaoka, K & Yonetoku, D 2001, 'Achievements of the ASTRO-E hard X-ray detector development', Paper presented at 2001 IEEE Nuclear Science Symposium Conference Record, San Diege, CA, United States, 4/11/01 - 10/11/01 pp. 483-486.

TY - CONF

T1 - Achievements of the ASTRO-E hard X-ray detector development

AU - Tashiro, M.

AU - Makishima, K.

AU - Kamae, T.

AU - Murakami, T.

AU - Takahashi, T.

AU - Fukazawa, Y.

AU - Kokubun, M.

AU - Nakazawa, K.

AU - Nomachi, M.

AU - Yoshida, A.

AU - Ezoe, Y.

AU - Isobe, N.

AU - Iyomoto, N.

AU - Kataoka, J.

AU - Kotoku, J.

AU - Kouda, M.

AU - Kubo, S.

AU - Kubota, A.

AU - Matsumoto, Y.

AU - Mizuno, T.

AU - Okada, Y.

AU - Ota, N.

AU - Ozawa, H.

AU - Sato, G.

AU - Sugiho, M.

AU - Sugizaki, M.

AU - Takahashi, I.

AU - Takahashi, H.

AU - Tamura, T.

AU - Tanihata, C.

AU - Terada, Y.

AU - Uchiyama, Y.

AU - Watanabe, S.

AU - Yamaoka, K.

AU - Yonetoku, D.

PY - 2001

Y1 - 2001

N2 - The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10-5 counts s-1cm-2keV-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.

AB - The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10-5 counts s-1cm-2keV-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.

KW - ASTRO-E

KW - Hard X-ray detector

KW - Sensitivity

KW - Spectral response

UR - https://www.scopus.com/pages/publications/0035553511

M3 - 論文

AN - SCOPUS:0035553511

SP - 483

EP - 486

T2 - 2001 IEEE Nuclear Science Symposium Conference Record

Y2 - 4 November 2001 through 10 November 2001

ER -

Achievements of the ASTRO-E hard X-ray detector development

Abstract

Conference

Keywords

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