Development and performance of the advanced hard x-ray telescope for the balloon experiment

Takuya Miyazawa; Ryo Shibata; Yasushi Ogasaka; Yoshihiro Fukaya; Masataka Naitou; Tomonaga Iwahara; Kenta Shimoda; Keisuke Tamura; Akihiro Furuzawa; Hideyo Kunieda; Koujun Yamashita; Shin Yokoi; Takuma Yoshii; Naoya Watanabe; Yoshiharu Namba

doi:10.1117/12.671346

Development and performance of the advanced hard x-ray telescope for the balloon experiment

Takuya Miyazawa, Ryo Shibata, Yasushi Ogasaka, Yoshihiro Fukaya, Masataka Naitou, Tomonaga Iwahara, Kenta Shimoda, Keisuke Tamura, Akihiro Furuzawa, Hideyo Kunieda, Koujun Yamashita, Shin Yokoi, Takuma Yoshii, Naoya Watanabe, Yoshiharu Namba

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

10 Citations (Scopus)

Abstract

Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.

Original language	English
Title of host publication	Space Telescopes and Instrumentation II
Subtitle of host publication	Ultraviolet to Gamma Ray
Volume	6266 II
DOIs	https://doi.org/10.1117/12.671346
Publication status	Published - 02-10-2006
Externally published	Yes
Event	Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray - Orlando, FL, United States Duration: 24-05-2006 → 31-05-2006

Other

Other	Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray
Country	United States
City	Orlando, FL
Period	24-05-06 → 31-05-06

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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Miyazawa, T., Shibata, R., Ogasaka, Y., Fukaya, Y., Naitou, M., Iwahara, T., Shimoda, K., Tamura, K., Furuzawa, A., Kunieda, H., Yamashita, K., Yokoi, S., Yoshii, T., Watanabe, N., & Namba, Y. (2006). Development and performance of the advanced hard x-ray telescope for the balloon experiment. In Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray (Vol. 6266 II). [62663C] https://doi.org/10.1117/12.671346

Miyazawa, Takuya ; Shibata, Ryo ; Ogasaka, Yasushi ; Fukaya, Yoshihiro ; Naitou, Masataka ; Iwahara, Tomonaga ; Shimoda, Kenta ; Tamura, Keisuke ; Furuzawa, Akihiro ; Kunieda, Hideyo ; Yamashita, Koujun ; Yokoi, Shin ; Yoshii, Takuma ; Watanabe, Naoya ; Namba, Yoshiharu. / Development and performance of the advanced hard x-ray telescope for the balloon experiment. Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. Vol. 6266 II 2006.

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title = "Development and performance of the advanced hard x-ray telescope for the balloon experiment",

abstract = "Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.",

author = "Takuya Miyazawa and Ryo Shibata and Yasushi Ogasaka and Yoshihiro Fukaya and Masataka Naitou and Tomonaga Iwahara and Kenta Shimoda and Keisuke Tamura and Akihiro Furuzawa and Hideyo Kunieda and Koujun Yamashita and Shin Yokoi and Takuma Yoshii and Naoya Watanabe and Yoshiharu Namba",

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doi = "10.1117/12.671346",

language = "English",

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Miyazawa, T, Shibata, R, Ogasaka, Y, Fukaya, Y, Naitou, M, Iwahara, T, Shimoda, K, Tamura, K, Furuzawa, A, Kunieda, H, Yamashita, K, Yokoi, S, Yoshii, T, Watanabe, N & Namba, Y 2006, Development and performance of the advanced hard x-ray telescope for the balloon experiment. in Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. vol. 6266 II, 62663C, Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray, Orlando, FL, United States, 24-05-06. https://doi.org/10.1117/12.671346

Development and performance of the advanced hard x-ray telescope for the balloon experiment. / Miyazawa, Takuya; Shibata, Ryo; Ogasaka, Yasushi; Fukaya, Yoshihiro; Naitou, Masataka; Iwahara, Tomonaga; Shimoda, Kenta; Tamura, Keisuke; Furuzawa, Akihiro; Kunieda, Hideyo; Yamashita, Koujun; Yokoi, Shin; Yoshii, Takuma; Watanabe, Naoya; Namba, Yoshiharu.

Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. Vol. 6266 II 2006. 62663C.

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

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T1 - Development and performance of the advanced hard x-ray telescope for the balloon experiment

AU - Miyazawa, Takuya

AU - Shibata, Ryo

AU - Ogasaka, Yasushi

AU - Fukaya, Yoshihiro

AU - Naitou, Masataka

AU - Iwahara, Tomonaga

AU - Shimoda, Kenta

AU - Tamura, Keisuke

AU - Furuzawa, Akihiro

AU - Kunieda, Hideyo

AU - Yamashita, Koujun

AU - Yokoi, Shin

AU - Yoshii, Takuma

AU - Watanabe, Naoya

AU - Namba, Yoshiharu

PY - 2006/10/2

Y1 - 2006/10/2

N2 - Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.

AB - Imaging observation in the hard X-ray band of 10 - 100 keV is one of the important subjects in X-ray astronomy. Though SUMIT balloon-borne experiment, we have developed thin-foil-nested hard X-ray telescope employing depth-graded Pt/C multilayer (multilayer-supermirror). We have improved production process of the replica reflector and telescope optics compared with InFOCμS-2004 telescope. The new telescope was measured at synchrotron radiation facility, SPring-8. The image quality and throughtput were estimated to be 2.06 arcmin (half power diameter) and 85 % at 30 keV, respectively. These values were about 24 % and 30 % improvement compared to InFOC/μS-2004, respectively. Limiting factors of its performance are also investigated. Based on such an investigation we are now continuously developing hard X-ray telescope for SUMIT 2006 flight.

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M3 - Conference contribution

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SN - 9780819463319

VL - 6266 II

BT - Space Telescopes and Instrumentation II

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

Y2 - 24 May 2006 through 31 May 2006

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