X-ray γ-ray Polarimetry Small Satellite PolariS

被引:1
|
作者
Hayashida, Kiyoshi [1 ]
Yonetoku, Daisuke
Gunji, Shuichi
Tamagawa, Toru
Mihara, Tatehiro
Mizuno, Tsunefumi
Dotani, Tadayasu
Kubo, Hidetoshi
Murakami, Toshio
Yatsu, Yoichi
Tokanai, Fuyuki
Sakurai, Hirohisa
Takahashi, Hiromitsu
Kitamoto, Shunji
Furuzawa, Akira
Sadamoto, Masaaki [1 ]
Kamitsukasa, Fumiyoshi [1 ]
Deguchi, Kazuhiro [1 ]
Anabuki, Naohisa [1 ]
Tsunemi, Hiroshi [1 ]
机构
[1] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan
来源
SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY | 2012年 / 8443卷
关键词
X-ray Polarimetry; PolariS; Small Satellite; PERFORMANCE;
D O I
10.1117/12.926002
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
PolariS (Polarimetry Satellite) is a Japanese small satellite mission dedicated to polarimetry of X-ray and gamma-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 gamma-ray polarimetry of transient sources, such as gamma-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.
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页数:9
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