Improvements of the Astro-E2 hard X-Ray Detector (HXD-II)

M. Kokubun; K. Abe; Y. Ezoe; Y. Fukazawa; S. Hong; H. Inoue; T. Itoh; T. Kamae; D. Kasama; M. Kawaharada; N. Kawano; K. Kawashima; S. Kawasoe; Y. Kobayashi; J. Kotoku; M. Kouda; A. Kubota; G. M. Madejski; K. Makishima; T. Mitani; H. Miyasaka; R. Miyawaki; K. Mori; M. Mori; T. Murakami; M. M. Murashima; K. Nakazawa; H. Niko; M. Nomachi; M. Ohno; Y. Okada; K. Oonuki; G. Sato; M. Suzuki; H. Takahashi; I. Takahashi; T. Takahashi; K. Tamura; T. Tanaka; M. Tashiro; Y. Terada; S. Tominaga; S. Watanabe; K. Yamaoka; T. Yanagida; D. Yonetoku

doi:10.1109/TNS.2004.832921

Improvements of the Astro-E2 hard X-Ray Detector (HXD-II)

M. Kokubun^*, K. Abe, Y. Ezoe, Y. Fukazawa, S. Hong, H. Inoue, T. Itoh, T. Kamae, D. Kasama, M. Kawaharada, N. Kawano, K. Kawashima, S. Kawasoe, Y. Kobayashi, J. Kotoku, M. Kouda, A. Kubota, G. M. Madejski, K. Makishima, T. MitaniH. Miyasaka, R. Miyawaki, K. Mori, M. Mori, T. Murakami, M. M. Murashima, K. Nakazawa, H. Niko, M. Nomachi, M. Ohno, Y. Okada, K. Oonuki, G. Sato, M. Suzuki, H. Takahashi, I. Takahashi, T. Takahashi, K. Tamura, T. Tanaka, M. Tashiro, Y. Terada, S. Tominaga, S. Watanabe, K. Yamaoka, T. Yanagida, D. Yonetoku

^*この研究の対応する著者

研究成果: Article › 査読

66 被引用数 (Scopus)

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We summarize significant improvements which have been achived in the development of Astro-E2 Hard X-ray Detector (HXD-II). An expanded energy range and better energy resolution have been achieved from progresses in device materials and re-designing of the front-end electronics. An improved estimation for the detector background in orbit has also been conducted based upon results from our proton irradiation experiment. The sensitivity of HXD-II can be expected to reach an order of 10^-6 [c s^-1 keV^-1 cm^-2].

本文言語	English
ページ（範囲）	1991-1996
ページ数	6
ジャーナル	IEEE Transactions on Nuclear Science
巻	51
号	5 I
DOI	https://doi.org/10.1109/TNS.2004.832921
出版ステータス	Published - 2004 10月

ASJC Scopus subject areas

電子工学および電気工学
原子力エネルギーおよび原子力工学

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10.1109/TNS.2004.832921

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Kokubun, M., Abe, K., Ezoe, Y., Fukazawa, Y., Hong, S., Inoue, H., Itoh, T., Kamae, T., Kasama, D., Kawaharada, M., Kawano, N., Kawashima, K., Kawasoe, S., Kobayashi, Y., Kotoku, J., Kouda, M., Kubota, A., Madejski, G. M., Makishima, K., ... Yonetoku, D. (2004). Improvements of the Astro-E2 hard X-Ray Detector (HXD-II). IEEE Transactions on Nuclear Science, 51(5 I), 1991-1996. https://doi.org/10.1109/TNS.2004.832921

Kokubun, M, Abe, K, Ezoe, Y, Fukazawa, Y, Hong, S, Inoue, H, Itoh, T, Kamae, T, Kasama, D, Kawaharada, M, Kawano, N, Kawashima, K, Kawasoe, S, Kobayashi, Y, Kotoku, J, Kouda, M, Kubota, A, Madejski, GM, Makishima, K, Mitani, T, Miyasaka, H, Miyawaki, R, Mori, K, Mori, M, Murakami, T, Murashima, MM, Nakazawa, K, Niko, H, Nomachi, M, Ohno, M, Okada, Y, Oonuki, K, Sato, G, Suzuki, M, Takahashi, H, Takahashi, I, Takahashi, T, Tamura, K, Tanaka, T, Tashiro, M, Terada, Y, Tominaga, S, Watanabe, S, Yamaoka, K, Yanagida, T & Yonetoku, D 2004, 'Improvements of the Astro-E2 hard X-Ray Detector (HXD-II)', IEEE Transactions on Nuclear Science, vol. 51, no. 5 I, pp. 1991-1996. https://doi.org/10.1109/TNS.2004.832921

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abstract = "We summarize significant improvements which have been achived in the development of Astro-E2 Hard X-ray Detector (HXD-II). An expanded energy range and better energy resolution have been achieved from progresses in device materials and re-designing of the front-end electronics. An improved estimation for the detector background in orbit has also been conducted based upon results from our proton irradiation experiment. The sensitivity of HXD-II can be expected to reach an order of 10-6 [c s-1 keV-1 cm-2].",

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author = "M. Kokubun and K. Abe and Y. Ezoe and Y. Fukazawa and S. Hong and H. Inoue and T. Itoh and T. Kamae and D. Kasama and M. Kawaharada and N. Kawano and K. Kawashima and S. Kawasoe and Y. Kobayashi and J. Kotoku and M. Kouda and A. Kubota and Madejski, {G. M.} and K. Makishima and T. Mitani and H. Miyasaka and R. Miyawaki and K. Mori and M. Mori and T. Murakami and Murashima, {M. M.} and K. Nakazawa and H. Niko and M. Nomachi and M. Ohno and Y. Okada and K. Oonuki and G. Sato and M. Suzuki and H. Takahashi and I. Takahashi and T. Takahashi and K. Tamura and T. Tanaka and M. Tashiro and Y. Terada and S. Tominaga and S. Watanabe and K. Yamaoka and T. Yanagida and D. Yonetoku",

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T1 - Improvements of the Astro-E2 hard X-Ray Detector (HXD-II)

AU - Kokubun, M.

AU - Abe, K.

AU - Ezoe, Y.

AU - Fukazawa, Y.

AU - Hong, S.

AU - Inoue, H.

AU - Itoh, T.

AU - Kamae, T.

AU - Kasama, D.

AU - Kawaharada, M.

AU - Kawano, N.

AU - Kawashima, K.

AU - Kawasoe, S.

AU - Kobayashi, Y.

AU - Kotoku, J.

AU - Kouda, M.

AU - Kubota, A.

AU - Madejski, G. M.

AU - Makishima, K.

AU - Mitani, T.

AU - Miyasaka, H.

AU - Miyawaki, R.

AU - Mori, K.

AU - Mori, M.

AU - Murakami, T.

AU - Murashima, M. M.

AU - Nakazawa, K.

AU - Niko, H.

AU - Nomachi, M.

AU - Ohno, M.

AU - Okada, Y.

AU - Oonuki, K.

AU - Sato, G.

AU - Suzuki, M.

AU - Takahashi, H.

AU - Takahashi, I.

AU - Takahashi, T.

AU - Tamura, K.

AU - Tanaka, T.

AU - Tashiro, M.

AU - Terada, Y.

AU - Tominaga, S.

AU - Watanabe, S.

AU - Yamaoka, K.

AU - Yanagida, T.

AU - Yonetoku, D.

PY - 2004/10

Y1 - 2004/10

N2 - We summarize significant improvements which have been achived in the development of Astro-E2 Hard X-ray Detector (HXD-II). An expanded energy range and better energy resolution have been achieved from progresses in device materials and re-designing of the front-end electronics. An improved estimation for the detector background in orbit has also been conducted based upon results from our proton irradiation experiment. The sensitivity of HXD-II can be expected to reach an order of 10-6 [c s-1 keV-1 cm-2].

AB - We summarize significant improvements which have been achived in the development of Astro-E2 Hard X-ray Detector (HXD-II). An expanded energy range and better energy resolution have been achieved from progresses in device materials and re-designing of the front-end electronics. An improved estimation for the detector background in orbit has also been conducted based upon results from our proton irradiation experiment. The sensitivity of HXD-II can be expected to reach an order of 10-6 [c s-1 keV-1 cm-2].

KW - γ-ray

KW - Astro-E2

KW - Astrophysics

KW - Detector

KW - Hard X-ray

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SP - 1991

EP - 1996

JO - IEEE Transactions on Nuclear Science

JF - IEEE Transactions on Nuclear Science

SN - 0018-9499

IS - 5 I

ER -

Improvements of the Astro-E2 hard X-Ray Detector (HXD-II)

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