Thin-foil multilayer-supermirror hard X-ray telescope for InFOC μS/SUMIT balloon exeriments and NeXT satellite program

Yasushi Ogasaka; Keisuke Tamura; Takuya Miyazawa; Yoshihiro Fukaya; Tomonaga Iwahara; Naoki Sasaki; Akihiro Furuzawa; Yoshito Haba; Yasufumi Kanou; Daisuke Ueno; Hideyo Kunieda; Koujun Yamashita; Ryo Shibata; Takashi Okajima; Jack Tueller; Peter Serlemitsos; Yang Soong; Kai Wing Chan; Emi Miyata; Hiroshi Tsunemi; Kentaro Uesugi; Yoshio Suzuki; Yoshiharu Namba

doi:10.1117/12.733694

Thin-foil multilayer-supermirror hard X-ray telescope for InFOC _μS/SUMIT balloon exeriments and NeXT satellite program

Yasushi Ogasaka, Keisuke Tamura, Takuya Miyazawa, Yoshihiro Fukaya, Tomonaga Iwahara, Naoki Sasaki, Akihiro Furuzawa, Yoshito Haba, Yasufumi Kanou, Daisuke Ueno, Hideyo Kunieda, Koujun Yamashita, Ryo Shibata, Takashi Okajima, Jack Tueller, Peter Serlemitsos, Yang Soong, Kai Wing Chan, Emi Miyata, Hiroshi TsunemiKentaro Uesugi, Yoshio Suzuki, Yoshiharu Namba

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

23 Citations (Scopus)

Abstract

Hard X-ray telescopes using depth-graded multilayer is a key technology for future satellite programs. Developments are underway by many groups, and balloon experiments have also been carried out. We have developed light-weight hard X-ray telescopes using Pt/C multilayer and high-throughput thin-foil optics. They have been aboard on InFOC_μS and SUMIT balloon flights. As a next development efforts, especially for Japan's NeXT satellite program, we focus on improvement of image quality. Among three equally-contributing error factors (figure error, positioning error and off-roundness), figure errors and off-roundness have been reduced significantly, by screening of replication mandrels and active and iterative tuning of support bars. Further studies are in progress, such as suer-polished metal mandrels and better positioning of reflector edges, to meet the baseline requirement of the NeXT mission.

Original language	English
Title of host publication	Optics for EUV, X-Ray, and Gamma-Ray Astronomy III
DOIs	https://doi.org/10.1117/12.733694
Publication status	Published - 2007
Externally published	Yes
Event	Optics for EUV, X-Ray, and Gamma-Ray Astronomy III - San Diego, CA, United States Duration: 29-08-2007 → 30-08-2007

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	6688
ISSN (Print)	0277-786X

Other

Other	Optics for EUV, X-Ray, and Gamma-Ray Astronomy III
Country/Territory	United States
City	San Diego, CA
Period	29-08-07 → 30-08-07

All Science Journal Classification (ASJC) codes

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

Access to Document

10.1117/12.733694

Cite this

Ogasaka, Y., Tamura, K., Miyazawa, T., Fukaya, Y., Iwahara, T., Sasaki, N., Furuzawa, A., Haba, Y., Kanou, Y., Ueno, D., Kunieda, H., Yamashita, K., Shibata, R., Okajima, T., Tueller, J., Serlemitsos, P., Soong, Y., Chan, K. W., Miyata, E., ... Namba, Y. (2007). Thin-foil multilayer-supermirror hard X-ray telescope for InFOC _μS/SUMIT balloon exeriments and NeXT satellite program. In Optics for EUV, X-Ray, and Gamma-Ray Astronomy III Article 668803 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6688). https://doi.org/10.1117/12.733694

@inproceedings{7d979e80894341edb37137be677fe0dc,

title = "Thin-foil multilayer-supermirror hard X-ray telescope for InFOC μS/SUMIT balloon exeriments and NeXT satellite program",

abstract = "Hard X-ray telescopes using depth-graded multilayer is a key technology for future satellite programs. Developments are underway by many groups, and balloon experiments have also been carried out. We have developed light-weight hard X-ray telescopes using Pt/C multilayer and high-throughput thin-foil optics. They have been aboard on InFOCμS and SUMIT balloon flights. As a next development efforts, especially for Japan's NeXT satellite program, we focus on improvement of image quality. Among three equally-contributing error factors (figure error, positioning error and off-roundness), figure errors and off-roundness have been reduced significantly, by screening of replication mandrels and active and iterative tuning of support bars. Further studies are in progress, such as suer-polished metal mandrels and better positioning of reflector edges, to meet the baseline requirement of the NeXT mission.",

author = "Yasushi Ogasaka and Keisuke Tamura and Takuya Miyazawa and Yoshihiro Fukaya and Tomonaga Iwahara and Naoki Sasaki and Akihiro Furuzawa and Yoshito Haba and Yasufumi Kanou and Daisuke Ueno and Hideyo Kunieda and Koujun Yamashita and Ryo Shibata and Takashi Okajima and Jack Tueller and Peter Serlemitsos and Yang Soong and Chan, {Kai Wing} and Emi Miyata and Hiroshi Tsunemi and Kentaro Uesugi and Yoshio Suzuki and Yoshiharu Namba",

year = "2007",

doi = "10.1117/12.733694",

language = "English",

isbn = "9780819468369",

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

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

note = "Optics for EUV, X-Ray, and Gamma-Ray Astronomy III ; Conference date: 29-08-2007 Through 30-08-2007",

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Ogasaka, Y, Tamura, K, Miyazawa, T, Fukaya, Y, Iwahara, T, Sasaki, N, Furuzawa, A, Haba, Y, Kanou, Y, Ueno, D, Kunieda, H, Yamashita, K, Shibata, R, Okajima, T, Tueller, J, Serlemitsos, P, Soong, Y, Chan, KW, Miyata, E, Tsunemi, H, Uesugi, K, Suzuki, Y & Namba, Y 2007, Thin-foil multilayer-supermirror hard X-ray telescope for InFOC _μS/SUMIT balloon exeriments and NeXT satellite program. in Optics for EUV, X-Ray, and Gamma-Ray Astronomy III., 668803, Proceedings of SPIE - The International Society for Optical Engineering, vol. 6688, Optics for EUV, X-Ray, and Gamma-Ray Astronomy III, San Diego, CA, United States, 29-08-07. https://doi.org/10.1117/12.733694

Thin-foil multilayer-supermirror hard X-ray telescope for InFOC _μS/SUMIT balloon exeriments and NeXT satellite program. / Ogasaka, Yasushi; Tamura, Keisuke; Miyazawa, Takuya et al.
Optics for EUV, X-Ray, and Gamma-Ray Astronomy III. 2007. 668803 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6688).

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

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T1 - Thin-foil multilayer-supermirror hard X-ray telescope for InFOC μS/SUMIT balloon exeriments and NeXT satellite program

AU - Ogasaka, Yasushi

AU - Tamura, Keisuke

AU - Miyazawa, Takuya

AU - Fukaya, Yoshihiro

AU - Iwahara, Tomonaga

AU - Sasaki, Naoki

AU - Furuzawa, Akihiro

AU - Haba, Yoshito

AU - Kanou, Yasufumi

AU - Ueno, Daisuke

AU - Kunieda, Hideyo

AU - Yamashita, Koujun

AU - Shibata, Ryo

AU - Okajima, Takashi

AU - Tueller, Jack

AU - Serlemitsos, Peter

AU - Soong, Yang

AU - Chan, Kai Wing

AU - Miyata, Emi

AU - Tsunemi, Hiroshi

AU - Uesugi, Kentaro

AU - Suzuki, Yoshio

AU - Namba, Yoshiharu

PY - 2007

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AB - Hard X-ray telescopes using depth-graded multilayer is a key technology for future satellite programs. Developments are underway by many groups, and balloon experiments have also been carried out. We have developed light-weight hard X-ray telescopes using Pt/C multilayer and high-throughput thin-foil optics. They have been aboard on InFOCμS and SUMIT balloon flights. As a next development efforts, especially for Japan's NeXT satellite program, we focus on improvement of image quality. Among three equally-contributing error factors (figure error, positioning error and off-roundness), figure errors and off-roundness have been reduced significantly, by screening of replication mandrels and active and iterative tuning of support bars. Further studies are in progress, such as suer-polished metal mandrels and better positioning of reflector edges, to meet the baseline requirement of the NeXT mission.

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