Characterization of a hard x-ray telescope at synchrotron facility SPring-8

被引:29
作者
Ogasaka, Yasushi [1 ]
Tamura, Keisuke [1 ]
Shibata, Ryo [1 ]
Furuzawa, Akihiro [1 ]
Miyazawa, Takuya [1 ]
Shimoda, Kenta [1 ]
Fukaya, Yoshihiro [1 ]
Iwahara, Tomonaga [1 ]
Nakamura, Tornokazu [1 ]
Naitou, Masataka [1 ]
Kanou, Yasufumi [1 ]
Sasaki, Naoki [1 ]
Ueno, Daislike [1 ]
Okajima, Takashi [2 ]
Miyata, Emi [3 ]
Tawa, Noriaki [3 ]
Mukai, Kenji [3 ]
Ikegami, Kazuhiro [3 ]
Aono, Michihiko [3 ]
Uesugi, Kentaro [4 ]
Suzuki, Yoshio [4 ]
Takeuchi, Satoshi [1 ]
Furamura, Taku [1 ]
Takahashi, Rika [1 ]
Sakashita, Machiko [1 ]
Sakai, Chiaki [1 ]
Nonoyama, Masayuki [1 ]
Yamada, Nobuaki [1 ]
Onishi, Katsuhiko [1 ]
Miyauchi, Tomofumi [3 ]
Maeda, Yoshitomo [5 ]
Okada, Shunsaku [5 ]
Serlemitsos, Peter [2 ]
Soong, Yang [2 ]
Chan, Kai-Wing [2 ]
Rohrbach, Scott [2 ]
Berendse, Fred [6 ]
Tueller, Jack [2 ]
Tsunemi, Hiroshi
Kunieda, Hideyo [1 ]
Yamashita, Koujun [1 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Osaka Univ, Dept Phys, Osaka 5600043, Japan
[4] Japan Synchrotron Radiat Res Inst, Sayou, Hyogo 6795198, Japan
[5] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[6] USN, Res Lab, Washington, DC 20375 USA
关键词
X-ray optics; X-ray telescope; synchrotron radiation; multilayer; measurement technique; space science; astronomy;
D O I
10.1143/JJAP.47.5743
中图分类号
O59 [应用物理学];
学科分类号
摘要
Space-borne astronomical instruments require extensive characterization on the ground before launch. In the hard X-ray region however, it is difficult for a laboratory-based beamline using a conventional X-ray Source to provide a capability sufficient for pre-flight high-precision calibration. In this paper, we describe an experiment to characterize a hard X-ray telescope at a synchrotron facility, mainly on the basis of experimental setup and examples of measured results. We have developed hard X-ray telescopes consisting of Wolter-I grazing incidence optics and platinum-carbon multilayer supermirror coatings. The telescopes have been characterized at the synchrotron facility SPring-8 beamline BL20B2. The measurements at BL20B2 have great advantages such as extremely high flux, large-sized and less-divergent beam, and monochromatic beam covering the entire hard X-ray region front 8 to over 100keV. The telescope was illuminated by monochromatic hard X-rays, and the focused image was measured by high resolution hard X-ray imagers. The entire telescope aperture was mapped by a small beam, and the effective area and the point spread function were obtained as well as local optical properties for further diagnostics of the characteristics of the telescope.
引用
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页码:5743 / 5754
页数:12
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