ASTRO-H Hard X-ray Telescope (HXT)

Hisamitsu Awaki, Hideyo Kunieda, Akihiro Furuzawa, Yoshito Haba, Takayuki Hayashi, Ryo Iizuka, Kazunori Ishibashi, Manabu Ishida, Masayuki Itoh, Tatsuro Kosaka, Yoshitomo Maeda, Hironori Matsumoto, Takuya Miyazawa, Hideyuki Mori, Hosei Nagano, Yoshiharu Namba, Yasushi Ogasaka, Keiji Ogi, Takashi Okajima, Satoshi SugitaYoshio Suzuki, Keisuke Tamura, Yuzuru Tawara, Kentaro Uesugi, Koujun Yamashita, Shigeo Yamauchi

研究成果: Conference contribution

12 引用 (Scopus)

抄録

The new Japanese X-ray Astronomy satellite, ASTRO-H will carry two identical hard X-ray telescopes (HXTs), which cover 5 to 80 keV, in order to provide new insights into frontier of X-ray astronomy. The HXT mirror surfaces are coated with Pt/C depth-graded multilayers to enhance hard X-ray effective area by means of Bragg reflection, and 213 mirror reflectors with a thickness of 0.22 mm are tightly nested confocally in a telescope. The production of FM HXT-1 and HXT-2 were completed in 2012 and 2013, respectively. The X-ray performance of HXTs were measured at the synchrotron radiation facility SPring-8/ BL20B2 Japan. The total effective area of two HXTs is about 350 cm2 at 30 keV and the angular resolution of HXT is about 1.'9 in half power diameter at 30 keV. The HXTs are in the clean room at ISAS for waiting the final integration test.

元の言語English
ホスト出版物のタイトルSpace Telescopes and Instrumentation 2014
ホスト出版物のサブタイトルUltraviolet to Gamma Ray
編集者Tadayuki Takahashi, Jan-Willem A. den Herder, Mark Bautz
出版者SPIE
ISBN(電子版)9780819496126
DOI
出版物ステータスPublished - 01-01-2014
外部発表Yes
イベントSpace Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray - Montreal, Canada
継続期間: 22-06-201426-06-2014

出版物シリーズ

名前Proceedings of SPIE - The International Society for Optical Engineering
9144
ISSN(印刷物)0277-786X
ISSN(電子版)1996-756X

Other

OtherSpace Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Canada
Montreal
期間22-06-1426-06-14

Fingerprint

X-ray Telescopes
Hard X-ray
Telescopes
telescopes
X rays
x rays
X-ray Astronomy
Astronomy
Mirror
astronomy
Synchrotron Radiation
Mirrors
Reflector
mirrors
clean rooms
Clean rooms
Japan
Telescope
Multilayer
angular resolution

All Science Journal Classification (ASJC) codes

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

これを引用

Awaki, H., Kunieda, H., Furuzawa, A., Haba, Y., Hayashi, T., Iizuka, R., ... Yamauchi, S. (2014). ASTRO-H Hard X-ray Telescope (HXT). : T. Takahashi, J-W. A. den Herder, & M. Bautz (版), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray [914426] (Proceedings of SPIE - The International Society for Optical Engineering; 巻数 9144). SPIE. https://doi.org/10.1117/12.2054633
Awaki, Hisamitsu ; Kunieda, Hideyo ; Furuzawa, Akihiro ; Haba, Yoshito ; Hayashi, Takayuki ; Iizuka, Ryo ; Ishibashi, Kazunori ; Ishida, Manabu ; Itoh, Masayuki ; Kosaka, Tatsuro ; Maeda, Yoshitomo ; Matsumoto, Hironori ; Miyazawa, Takuya ; Mori, Hideyuki ; Nagano, Hosei ; Namba, Yoshiharu ; Ogasaka, Yasushi ; Ogi, Keiji ; Okajima, Takashi ; Sugita, Satoshi ; Suzuki, Yoshio ; Tamura, Keisuke ; Tawara, Yuzuru ; Uesugi, Kentaro ; Yamashita, Koujun ; Yamauchi, Shigeo. / ASTRO-H Hard X-ray Telescope (HXT). Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. 編集者 / Tadayuki Takahashi ; Jan-Willem A. den Herder ; Mark Bautz. SPIE, 2014. (Proceedings of SPIE - The International Society for Optical Engineering).
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abstract = "The new Japanese X-ray Astronomy satellite, ASTRO-H will carry two identical hard X-ray telescopes (HXTs), which cover 5 to 80 keV, in order to provide new insights into frontier of X-ray astronomy. The HXT mirror surfaces are coated with Pt/C depth-graded multilayers to enhance hard X-ray effective area by means of Bragg reflection, and 213 mirror reflectors with a thickness of 0.22 mm are tightly nested confocally in a telescope. The production of FM HXT-1 and HXT-2 were completed in 2012 and 2013, respectively. The X-ray performance of HXTs were measured at the synchrotron radiation facility SPring-8/ BL20B2 Japan. The total effective area of two HXTs is about 350 cm2 at 30 keV and the angular resolution of HXT is about 1.'9 in half power diameter at 30 keV. The HXTs are in the clean room at ISAS for waiting the final integration test.",
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Awaki, H, Kunieda, H, Furuzawa, A, Haba, Y, Hayashi, T, Iizuka, R, Ishibashi, K, Ishida, M, Itoh, M, Kosaka, T, Maeda, Y, Matsumoto, H, Miyazawa, T, Mori, H, Nagano, H, Namba, Y, Ogasaka, Y, Ogi, K, Okajima, T, Sugita, S, Suzuki, Y, Tamura, K, Tawara, Y, Uesugi, K, Yamashita, K & Yamauchi, S 2014, ASTRO-H Hard X-ray Telescope (HXT). : T Takahashi, J-WA den Herder & M Bautz (版), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray., 914426, Proceedings of SPIE - The International Society for Optical Engineering, 巻. 9144, SPIE, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, Montreal, Canada, 22-06-14. https://doi.org/10.1117/12.2054633

ASTRO-H Hard X-ray Telescope (HXT). / Awaki, Hisamitsu; Kunieda, Hideyo; Furuzawa, Akihiro; Haba, Yoshito; Hayashi, Takayuki; Iizuka, Ryo; Ishibashi, Kazunori; Ishida, Manabu; Itoh, Masayuki; Kosaka, Tatsuro; Maeda, Yoshitomo; Matsumoto, Hironori; Miyazawa, Takuya; Mori, Hideyuki; Nagano, Hosei; Namba, Yoshiharu; Ogasaka, Yasushi; Ogi, Keiji; Okajima, Takashi; Sugita, Satoshi; Suzuki, Yoshio; Tamura, Keisuke; Tawara, Yuzuru; Uesugi, Kentaro; Yamashita, Koujun; Yamauchi, Shigeo.

Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. 版 / Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz. SPIE, 2014. 914426 (Proceedings of SPIE - The International Society for Optical Engineering; 巻 9144).

研究成果: Conference contribution

TY - GEN

T1 - ASTRO-H Hard X-ray Telescope (HXT)

AU - Awaki, Hisamitsu

AU - Kunieda, Hideyo

AU - Furuzawa, Akihiro

AU - Haba, Yoshito

AU - Hayashi, Takayuki

AU - Iizuka, Ryo

AU - Ishibashi, Kazunori

AU - Ishida, Manabu

AU - Itoh, Masayuki

AU - Kosaka, Tatsuro

AU - Maeda, Yoshitomo

AU - Matsumoto, Hironori

AU - Miyazawa, Takuya

AU - Mori, Hideyuki

AU - Nagano, Hosei

AU - Namba, Yoshiharu

AU - Ogasaka, Yasushi

AU - Ogi, Keiji

AU - Okajima, Takashi

AU - Sugita, Satoshi

AU - Suzuki, Yoshio

AU - Tamura, Keisuke

AU - Tawara, Yuzuru

AU - Uesugi, Kentaro

AU - Yamashita, Koujun

AU - Yamauchi, Shigeo

PY - 2014/1/1

Y1 - 2014/1/1

N2 - The new Japanese X-ray Astronomy satellite, ASTRO-H will carry two identical hard X-ray telescopes (HXTs), which cover 5 to 80 keV, in order to provide new insights into frontier of X-ray astronomy. The HXT mirror surfaces are coated with Pt/C depth-graded multilayers to enhance hard X-ray effective area by means of Bragg reflection, and 213 mirror reflectors with a thickness of 0.22 mm are tightly nested confocally in a telescope. The production of FM HXT-1 and HXT-2 were completed in 2012 and 2013, respectively. The X-ray performance of HXTs were measured at the synchrotron radiation facility SPring-8/ BL20B2 Japan. The total effective area of two HXTs is about 350 cm2 at 30 keV and the angular resolution of HXT is about 1.'9 in half power diameter at 30 keV. The HXTs are in the clean room at ISAS for waiting the final integration test.

AB - The new Japanese X-ray Astronomy satellite, ASTRO-H will carry two identical hard X-ray telescopes (HXTs), which cover 5 to 80 keV, in order to provide new insights into frontier of X-ray astronomy. The HXT mirror surfaces are coated with Pt/C depth-graded multilayers to enhance hard X-ray effective area by means of Bragg reflection, and 213 mirror reflectors with a thickness of 0.22 mm are tightly nested confocally in a telescope. The production of FM HXT-1 and HXT-2 were completed in 2012 and 2013, respectively. The X-ray performance of HXTs were measured at the synchrotron radiation facility SPring-8/ BL20B2 Japan. The total effective area of two HXTs is about 350 cm2 at 30 keV and the angular resolution of HXT is about 1.'9 in half power diameter at 30 keV. The HXTs are in the clean room at ISAS for waiting the final integration test.

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M3 - Conference contribution

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T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2014

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A2 - den Herder, Jan-Willem A.

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Awaki H, Kunieda H, Furuzawa A, Haba Y, Hayashi T, Iizuka R その他. ASTRO-H Hard X-ray Telescope (HXT). : Takahashi T, den Herder J-WA, Bautz M, 編集者, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. SPIE. 2014. 914426. (Proceedings of SPIE - The International Society for Optical Engineering). https://doi.org/10.1117/12.2054633