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.

引用

页数：9

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