27 September 2012 X-ray gamma-ray polarimetry small satellite PolariS
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PolariS (Polarimetry Satellite) is a Japanese small satellite mission dedicated to polarimetry of X-ray and γ-ray sources. The primary aim of the mission is to perform wide band X-ray (4-80 keV) polarimetry of sources brighter than 10 mCrab. For this purpose, Polaris employs three hard X-ray telescopes and two types of focal plane imaging polarimeters. PolariS observations will measure the X-ray polarization for tens of sources including extragalactic ones mostly for the first time. The second purpose of the mission is γ-ray polarimetry of transient sources, such as γ-ray bursts. Wide field polarimeters based on similar concept as that used in the IKAROS/GAP but with higher sensitivity, i.e., polarization measurement of 10 bursts per year, will be employed.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kiyoshi Hayashida, Kiyoshi Hayashida, Daisuke Yonetoku, Daisuke Yonetoku, Shuichi Gunji, Shuichi Gunji, Toru Tamagawa, Toru Tamagawa, Tatehiro Mihara, Tatehiro Mihara, Tsunefumi Mizuno, Tsunefumi Mizuno, Tadayasu Dotani, Tadayasu Dotani, Hidetoshi Kubo, Hidetoshi Kubo, Toshio Murakami, Toshio Murakami, Yoichi Yatsu, Yoichi Yatsu, Fuyuki Tokanai, Fuyuki Tokanai, Hirohisa Sakurai, Hirohisa Sakurai, Hiromitsu Takahashi, Hiromitsu Takahashi, Shunji Kitamoto, Shunji Kitamoto, Akira Furuzawa, Akira Furuzawa, Masaaki Sadamoto, Masaaki Sadamoto, Fumiyoshi Kamitsukasa, Fumiyoshi Kamitsukasa, Kazuhiro Deguchi, Kazuhiro Deguchi, Naohisa Anabuki, Naohisa Anabuki, Hiroshi Tsunemi, Hiroshi Tsunemi, } "X-ray gamma-ray polarimetry small satellite PolariS", Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 84434G (27 September 2012); doi: 10.1117/12.926002; https://doi.org/10.1117/12.926002


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