Development of supermirror hard X-ray telescope and the results of the first InFOCuS flight observation

被引:21
作者
Ogasaka, Y [1 ]
Tamura, K [1 ]
Okajima, T [1 ]
Tawara, Y [1 ]
Yamashita, K [1 ]
Furuzawa, A [1 ]
Haga, K [1 ]
Ichimaru, S [1 ]
Takahashi, S [1 ]
Fukuda, S [1 ]
Kito, H [1 ]
Goto, A [1 ]
Kato, S [1 ]
Satake, H [1 ]
Nomoto, K [1 ]
Hamada, N [1 ]
Serlemitsos, PJ [1 ]
Tueller, J [1 ]
Soong, Y [1 ]
Chan, KW [1 ]
Owens, SM [1 ]
Berendse, FB [1 ]
Krimm, HA [1 ]
Baumgartner, W [1 ]
Barthelmy, SD [1 ]
Kunieda, H [1 ]
Misaki, K [1 ]
Shibata, R [1 ]
Mori, H [1 ]
Itoh, K [1 ]
Namba, Y [1 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
来源
X-RAY AND GAMMA-RAY TELESCOPES AND INSTRUMENTS FOR ASTRONOMY, PTS 1 AND 2 | 2003年 / 4851卷
关键词
X-ray telescope; hard X-ray telescope; multilayer; balloon observation; future mission;
D O I
10.1117/12.461531
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The development of hard X-ray focusing optics is widely recognized as one of key technologies for future X-ray observatory missions such as NeXT(Japan), Constellation-X(US) and possibly XEUS(Europe). We have developed hard X-ray telescope employing depth-graded multilayers, so-called supermirrors. Its benefit is to reflect hard X-rays by Bragg reflection at incidence angles larger than the critical angle of total external reflection. InFOCmuS is an international balloon-borne hard X-ray observation experiment initiated by NASA/GSFC. InFOCmuS hard X-ray telescope has been jointly developed by Nagoya University and GSFC. The telescope is conical approximation of Wolter-I optics with 8 m focal length and 40 cm diameter. It consists of 255 nested ultra-thin reflector pairs with incidence angles of 0.10 to 0.36 deg. Reflectors are coated with Pt/C supermirrors with periodic length of 2.9 to 13 nm and bi-layer number of 25 to 65, depending on incidence angles. The effective area and imaging quality are expected as 100 cm(2) in at 30 keV and 2 arcmin Half Power Diameter, respectively. The InFOCmuS experiment was launched on July 5, 2001, from National Scientific Balloon Facility in Texas, USA. We successfully observed Cyg X-1, chosen for a calibration target, in 20-40 keV energy band. We are planning to carry out next flight for scientific observations as soon as additional telescopes, detectors, and upgraded gondola system are implemented.
引用
收藏
页码:619 / 630
页数:12
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