The current status of ASTRO-H/HXT development facility

Akihiro Furuzawa; Yasushi Ogasaka; Hideyo Kunieda; Takuya Miyazawa; Masato Sakai; Yosuke Kinoshita; Youta Makinae; Shiori Sasaya; Yasufumi Kanou; Daisuke Niki; Takuya Ohgi; Nodoka Oishi; Koudai Yamane; Nobuyuki Yamane; Yosuke Ishida; Yoshito Haba; Yuzuru Tawara; Koujun Yamashita; Manabu Ishida; Yoshitomo Maeda; Hideyuki Mori; Keisuke Tamura; Hisamitsu Awaki; Takashi Okajima

doi:10.1117/12.825771

The current status of ASTRO-H/HXT development facility

Akihiro Furuzawa, Yasushi Ogasaka, Hideyo Kunieda, Takuya Miyazawa, Masato Sakai, Yosuke Kinoshita, Youta Makinae, Shiori Sasaya, Yasufumi Kanou, Daisuke Niki, Takuya Ohgi, Nodoka Oishi, Koudai Yamane, Nobuyuki Yamane, Yosuke Ishida, Yoshito Haba, Yuzuru Tawara, Koujun Yamashita, Manabu Ishida, Yoshitomo MaedaHideyuki Mori, Keisuke Tamura, Hisamitsu Awaki, Takashi Okajima

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

11 Citations (Scopus)

Abstract

We present the current state of the development system of the hard ray telescope onboard ASTRO-H satellite.Japan's 6th X-ray satellite mission ASTRO-H, which is planed to be launched in fiscal year 2013, will carry four X-ray telescopes (XRT). Two of four XRTs are hard X-ray telescopes (HXT) using depth-graded multilayer reflector which provide us the capability of hard X-ray imaging observation up to 80 keV. ASTRO-H/HXT is the light-weight hard X-ray telescope using Pt/C depth-graded multilayer and high-throughput thin-foil optics. The basic technology for fabricating the ASTRO-H/HXT has been established through the balloon borne experiments, "InFOCμS" (US-Japan international joint experiment) and "SUMIT" missions. (Nagoya University, Osaka University and JAXA). Major changes from XRTs onboard InFOCμS and SUMIT missions are large aperture size of 45 cm in diameter, the length of reflectors of 20 cm and the focal length of 12 m (XRTs onboard the balloon missions above have the aperture size of 40 cm in diameter, 13 cm long reflectors and 8 m focal length). Now we have almost finished to establish the mirror production facility dedicated to the ASTRO-H/HXT and are starting to produce foil reflectors for performance verification of 200 mm long reflector. We report the current status of the development facilities and test foil production.

Original language	English
Title of host publication	Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV
DOIs	https://doi.org/10.1117/12.825771
Publication status	Published - 2009
Externally published	Yes
Event	Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV - San Diego, CA, United States Duration: 04-08-2009 → 06-08-2009

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7437
ISSN (Print)	0277-786X

Other

Other	Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV
Country/Territory	United States
City	San Diego, CA
Period	04-08-09 → 06-08-09

All Science Journal Classification (ASJC) codes

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

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10.1117/12.825771

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Furuzawa, A., Ogasaka, Y., Kunieda, H., Miyazawa, T., Sakai, M., Kinoshita, Y., Makinae, Y., Sasaya, S., Kanou, Y., Niki, D., Ohgi, T., Oishi, N., Yamane, K., Yamane, N., Ishida, Y., Haba, Y., Tawara, Y., Yamashita, K., Ishida, M., ... Okajima, T. (2009). The current status of ASTRO-H/HXT development facility. In Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV [743709] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7437). https://doi.org/10.1117/12.825771

Furuzawa, Akihiro ; Ogasaka, Yasushi ; Kunieda, Hideyo ; Miyazawa, Takuya ; Sakai, Masato ; Kinoshita, Yosuke ; Makinae, Youta ; Sasaya, Shiori ; Kanou, Yasufumi ; Niki, Daisuke ; Ohgi, Takuya ; Oishi, Nodoka ; Yamane, Koudai ; Yamane, Nobuyuki ; Ishida, Yosuke ; Haba, Yoshito ; Tawara, Yuzuru ; Yamashita, Koujun ; Ishida, Manabu ; Maeda, Yoshitomo ; Mori, Hideyuki ; Tamura, Keisuke ; Awaki, Hisamitsu ; Okajima, Takashi. / The current status of ASTRO-H/HXT development facility. Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV. 2009. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{e64efd3600dd4264ac5ad50f9ba4849c,

title = "The current status of ASTRO-H/HXT development facility",

abstract = "We present the current state of the development system of the hard ray telescope onboard ASTRO-H satellite.Japan's 6th X-ray satellite mission ASTRO-H, which is planed to be launched in fiscal year 2013, will carry four X-ray telescopes (XRT). Two of four XRTs are hard X-ray telescopes (HXT) using depth-graded multilayer reflector which provide us the capability of hard X-ray imaging observation up to 80 keV. ASTRO-H/HXT is the light-weight hard X-ray telescope using Pt/C depth-graded multilayer and high-throughput thin-foil optics. The basic technology for fabricating the ASTRO-H/HXT has been established through the balloon borne experiments, {"}InFOCμS{"} (US-Japan international joint experiment) and {"}SUMIT{"} missions. (Nagoya University, Osaka University and JAXA). Major changes from XRTs onboard InFOCμS and SUMIT missions are large aperture size of 45 cm in diameter, the length of reflectors of 20 cm and the focal length of 12 m (XRTs onboard the balloon missions above have the aperture size of 40 cm in diameter, 13 cm long reflectors and 8 m focal length). Now we have almost finished to establish the mirror production facility dedicated to the ASTRO-H/HXT and are starting to produce foil reflectors for performance verification of 200 mm long reflector. We report the current status of the development facilities and test foil production.",

author = "Akihiro Furuzawa and Yasushi Ogasaka and Hideyo Kunieda and Takuya Miyazawa and Masato Sakai and Yosuke Kinoshita and Youta Makinae and Shiori Sasaya and Yasufumi Kanou and Daisuke Niki and Takuya Ohgi and Nodoka Oishi and Koudai Yamane and Nobuyuki Yamane and Yosuke Ishida and Yoshito Haba and Yuzuru Tawara and Koujun Yamashita and Manabu Ishida and Yoshitomo Maeda and Hideyuki Mori and Keisuke Tamura and Hisamitsu Awaki and Takashi Okajima",

year = "2009",

doi = "10.1117/12.825771",

language = "English",

isbn = "9780819477279",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV",

note = "Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV ; Conference date: 04-08-2009 Through 06-08-2009",

}

Furuzawa, A, Ogasaka, Y, Kunieda, H, Miyazawa, T, Sakai, M, Kinoshita, Y, Makinae, Y, Sasaya, S, Kanou, Y, Niki, D, Ohgi, T, Oishi, N, Yamane, K, Yamane, N, Ishida, Y, Haba, Y, Tawara, Y, Yamashita, K, Ishida, M, Maeda, Y, Mori, H, Tamura, K, Awaki, H & Okajima, T 2009, The current status of ASTRO-H/HXT development facility. in Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV., 743709, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7437, Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV, San Diego, CA, United States, 04-08-09. https://doi.org/10.1117/12.825771

The current status of ASTRO-H/HXT development facility. / Furuzawa, Akihiro; Ogasaka, Yasushi; Kunieda, Hideyo; Miyazawa, Takuya; Sakai, Masato; Kinoshita, Yosuke; Makinae, Youta; Sasaya, Shiori; Kanou, Yasufumi; Niki, Daisuke; Ohgi, Takuya; Oishi, Nodoka; Yamane, Koudai; Yamane, Nobuyuki; Ishida, Yosuke; Haba, Yoshito; Tawara, Yuzuru; Yamashita, Koujun; Ishida, Manabu; Maeda, Yoshitomo; Mori, Hideyuki; Tamura, Keisuke; Awaki, Hisamitsu; Okajima, Takashi.

Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV. 2009. 743709 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7437).

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

TY - GEN

T1 - The current status of ASTRO-H/HXT development facility

AU - Furuzawa, Akihiro

AU - Ogasaka, Yasushi

AU - Kunieda, Hideyo

AU - Miyazawa, Takuya

AU - Sakai, Masato

AU - Kinoshita, Yosuke

AU - Makinae, Youta

AU - Sasaya, Shiori

AU - Kanou, Yasufumi

AU - Niki, Daisuke

AU - Ohgi, Takuya

AU - Oishi, Nodoka

AU - Yamane, Koudai

AU - Yamane, Nobuyuki

AU - Ishida, Yosuke

AU - Haba, Yoshito

AU - Tawara, Yuzuru

AU - Yamashita, Koujun

AU - Ishida, Manabu

AU - Maeda, Yoshitomo

AU - Mori, Hideyuki

AU - Tamura, Keisuke

AU - Awaki, Hisamitsu

AU - Okajima, Takashi

PY - 2009

Y1 - 2009

N2 - We present the current state of the development system of the hard ray telescope onboard ASTRO-H satellite.Japan's 6th X-ray satellite mission ASTRO-H, which is planed to be launched in fiscal year 2013, will carry four X-ray telescopes (XRT). Two of four XRTs are hard X-ray telescopes (HXT) using depth-graded multilayer reflector which provide us the capability of hard X-ray imaging observation up to 80 keV. ASTRO-H/HXT is the light-weight hard X-ray telescope using Pt/C depth-graded multilayer and high-throughput thin-foil optics. The basic technology for fabricating the ASTRO-H/HXT has been established through the balloon borne experiments, "InFOCμS" (US-Japan international joint experiment) and "SUMIT" missions. (Nagoya University, Osaka University and JAXA). Major changes from XRTs onboard InFOCμS and SUMIT missions are large aperture size of 45 cm in diameter, the length of reflectors of 20 cm and the focal length of 12 m (XRTs onboard the balloon missions above have the aperture size of 40 cm in diameter, 13 cm long reflectors and 8 m focal length). Now we have almost finished to establish the mirror production facility dedicated to the ASTRO-H/HXT and are starting to produce foil reflectors for performance verification of 200 mm long reflector. We report the current status of the development facilities and test foil production.

AB - We present the current state of the development system of the hard ray telescope onboard ASTRO-H satellite.Japan's 6th X-ray satellite mission ASTRO-H, which is planed to be launched in fiscal year 2013, will carry four X-ray telescopes (XRT). Two of four XRTs are hard X-ray telescopes (HXT) using depth-graded multilayer reflector which provide us the capability of hard X-ray imaging observation up to 80 keV. ASTRO-H/HXT is the light-weight hard X-ray telescope using Pt/C depth-graded multilayer and high-throughput thin-foil optics. The basic technology for fabricating the ASTRO-H/HXT has been established through the balloon borne experiments, "InFOCμS" (US-Japan international joint experiment) and "SUMIT" missions. (Nagoya University, Osaka University and JAXA). Major changes from XRTs onboard InFOCμS and SUMIT missions are large aperture size of 45 cm in diameter, the length of reflectors of 20 cm and the focal length of 12 m (XRTs onboard the balloon missions above have the aperture size of 40 cm in diameter, 13 cm long reflectors and 8 m focal length). Now we have almost finished to establish the mirror production facility dedicated to the ASTRO-H/HXT and are starting to produce foil reflectors for performance verification of 200 mm long reflector. We report the current status of the development facilities and test foil production.

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U2 - 10.1117/12.825771

DO - 10.1117/12.825771

M3 - Conference contribution

AN - SCOPUS:70449432847

SN - 9780819477279

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

BT - Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV

T2 - Optics for EUV, X-Ray, and Gamma-Ray Astronomy IV

Y2 - 4 August 2009 through 6 August 2009

ER -

The current status of ASTRO-H/HXT development facility

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