Development of Pixel-Readout Micro-Pixel Chamber for X-ray Polarimetry
スポンサーリンク
概要
- 論文の詳細を見る
We developed a pixel-readout micro-pixel chamber ($\mu$-PIC) as an astronomical X-ray polarimeter and demonstrated its ability to achieve a higher sensitivity than a strip-readout one by a beam test. The $\mu$-PIC is one of the micropattern gas detectors that have been developed so far. However, its readout was of the strip type. This limits the sensitivity to polarization because it cannot determine the polarization angle uniquely without rotating the detector. Thus, we started developing the pixel-readout type of $\mu$-PIC. A beam test at a synchrotron-radiation facility was carried out to examine the performance for polarimetry. Without rotating the detector, we successfully detected the polarization angle. The modulation factor for 8 keV X-rays in a neon-based mixture was $0.12\pm 0.03$, which is at the same level as that of the strip-type $\mu$-PIC, and $0.07\pm 0.01$ at 15 keV in an argon-based mixture. These results indicate the ability of the new $\mu$-PIC to achieve a higher sensitivity to X-ray polarization than that obtainable with the strip-type $\mu$-PIC.
- 2007-05-15
著者
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Ueno Masaru
Department Of Chemistry Faculty Of Science Shizuoka University
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TSURU Takeshi
Cosmic Ray Group, Department of Physics, Kyoto University
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Ueno Masaru
Department of Physics, Faculty of Science, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
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Katagiri Hideaki
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Ono Kenichi
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Matsumoto Hironori
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Nagayoshi Tsutomu
Advanced Research Institute for Science and Engineering, 17 Kikui-cho, Shinjuku-ku, Tokyo 162-0044, Japan
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Hyodo Yosiaki
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Kubo Hidetoshi
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Miuchi Kentaro
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Tanimori Toru
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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Tsuru Takeshi
Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan
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