X-ray γ-ray polarimetry small satellite PolariS

Kiyoshi Hayashida; Daisuke Yonetoku; Shuichi Gunji; Toru Tamagawa; Tatehiro Mihara; Tsunefumi Mizuno; Hiromitsu Takahashi; Tadayasu Dotani; Hidetoshi Kubo; Yoichi Yatsu; Fuyuku Tokanai; Takeshi Nakamori; Shinpei Shibata; Asami Hayato; Akihiro Furuzawa; Yuji Kishimoto; Shunji Kitamoto; Kenji Toma; Masaaki Sadamoto; Keigo Yoshinaga; Juyong Kim; Shunichiro Ide; Fumiyoshi Kamitsukasa; Naohisa Anabuki; Hiroshi Tsunemi; Jun Katagiri; Juri Sugimoto

doi:10.1117/12.2056685

X-ray γ-ray polarimetry small satellite PolariS

Kiyoshi Hayashida
, Daisuke Yonetoku
, Shuichi Gunji
, Toru Tamagawa
, Tatehiro Mihara
, Tsunefumi Mizuno
, Hiromitsu Takahashi
, Tadayasu Dotani
, Hidetoshi Kubo
, Yoichi Yatsu
, Fuyuku Tokanai
, Takeshi Nakamori
, Shinpei Shibata
, Asami Hayato
, Akihiro Furuzawa
, Yuji Kishimoto
, Shunji Kitamoto
, Kenji Toma
, Masaaki Sadamoto
, Keigo Yoshinaga

Juyong Kim, Shunichiro Ide, Fumiyoshi Kamitsukasa, Naohisa Anabuki, Hiroshi Tsunemi, Jun Katagiri, Juri Sugimoto

研究成果: 書籍/レポートタイプへの寄稿 › 会議への寄与

8 被引用数 (Scopus)

抄録

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 hard X-ray (10-80 keV) polarimetry of sources brighter than 10 mCrab. For this purpose, PolariS employs three hard X-ray telescopes and scattering type imaging polarimeters. PolariS 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 (GRBs). Wide field polarimeters based on similar concept as that used in the IKAROS/GAP but with higher sensitivity will be used, and polarization measurement of 10 GRBs per year is expected.

本文言語	英語
ホスト出版物のタイトル	Space Telescopes and Instrumentation 2014
ホスト出版物のサブタイトル	Ultraviolet to Gamma Ray
編集者	Tadayuki Takahashi, Jan-Willem A. den Herder, Mark Bautz
出版社	SPIE
ISBN（電子版）	9780819496126
DOI	https://doi.org/10.1117/12.2056685
出版ステータス	出版済み - 2014
外部発表	はい
イベント	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray - Montreal, カナダ継続期間: 22-06-2014 → 26-06-2014

出版物シリーズ

名前	Proceedings of SPIE - The International Society for Optical Engineering
巻	9144
ISSN（印刷版）	0277-786X
ISSN（電子版）	1996-756X

その他

その他	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
国/地域	カナダ
City	Montreal
Period	22-06-14 → 26-06-14

All Science Journal Classification (ASJC) codes

電子材料、光学材料、および磁性材料
凝縮系物理学
コンピュータサイエンスの応用
応用数学
電子工学および電気工学

文献へのアクセス

10.1117/12.2056685

他のファイルとリンク

引用スタイル

Hayashida, K., Yonetoku, D., Gunji, S., Tamagawa, T., Mihara, T., Mizuno, T., Takahashi, H., Dotani, T., Kubo, H., Yatsu, Y., Tokanai, F., Nakamori, T., Shibata, S., Hayato, A., Furuzawa, A., Kishimoto, Y., Kitamoto, S., Toma, K., Sadamoto, M., ... Sugimoto, J. (2014). X-ray γ-ray polarimetry small satellite PolariS. In T. Takahashi, J.-W. A. den Herder, & M. Bautz (Eds.), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray 記事 91440K (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9144). SPIE. https://doi.org/10.1117/12.2056685

@inproceedings{62db90e5dc344ad09b3ce6f758009e75,

title = "X-ray γ-ray polarimetry small satellite PolariS",

abstract = "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 hard X-ray (10-80 keV) polarimetry of sources brighter than 10 mCrab. For this purpose, PolariS employs three hard X-ray telescopes and scattering type imaging polarimeters. PolariS 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 (GRBs). Wide field polarimeters based on similar concept as that used in the IKAROS/GAP but with higher sensitivity will be used, and polarization measurement of 10 GRBs per year is expected.",

keywords = "GRB, Hard X-ray, PolariS, Small Satellite, X-ray Polarimetry, X-ray Scattering",

author = "Kiyoshi Hayashida and Daisuke Yonetoku and Shuichi Gunji and Toru Tamagawa and Tatehiro Mihara and Tsunefumi Mizuno and Hiromitsu Takahashi and Tadayasu Dotani and Hidetoshi Kubo and Yoichi Yatsu and Fuyuku Tokanai and Takeshi Nakamori and Shinpei Shibata and Asami Hayato and Akihiro Furuzawa and Yuji Kishimoto and Shunji Kitamoto and Kenji Toma and Masaaki Sadamoto and Keigo Yoshinaga and Juyong Kim and Shunichiro Ide and Fumiyoshi Kamitsukasa and Naohisa Anabuki and Hiroshi Tsunemi and Jun Katagiri and Juri Sugimoto",

note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray ; Conference date: 22-06-2014 Through 26-06-2014",

year = "2014",

doi = "10.1117/12.2056685",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Tadayuki Takahashi and \{den Herder\}, \{Jan-Willem A.\} and Mark Bautz",

booktitle = "Space Telescopes and Instrumentation 2014",

address = "United States",

}

Hayashida, K, Yonetoku, D, Gunji, S, Tamagawa, T, Mihara, T, Mizuno, T, Takahashi, H, Dotani, T, Kubo, H, Yatsu, Y, Tokanai, F, Nakamori, T, Shibata, S, Hayato, A, Furuzawa, A, Kishimoto, Y, Kitamoto, S, Toma, K, Sadamoto, M, Yoshinaga, K, Kim, J, Ide, S, Kamitsukasa, F, Anabuki, N, Tsunemi, H, Katagiri, J & Sugimoto, J 2014, X-ray γ-ray polarimetry small satellite PolariS. in T Takahashi, J-WA den Herder & M Bautz (eds), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray., 91440K, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9144, SPIE, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, Montreal, カナダ, 22-06-14. https://doi.org/10.1117/12.2056685

X-ray γ-ray polarimetry small satellite PolariS. / Hayashida, Kiyoshi; Yonetoku, Daisuke; Gunji, Shuichi その他.
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. ed. / Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz. SPIE, 2014. 91440K (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9144).

研究成果: 書籍/レポートタイプへの寄稿 › 会議への寄与

TY - GEN

T1 - X-ray γ-ray polarimetry small satellite PolariS

AU - Hayashida, Kiyoshi

AU - Yonetoku, Daisuke

AU - Gunji, Shuichi

AU - Tamagawa, Toru

AU - Mihara, Tatehiro

AU - Mizuno, Tsunefumi

AU - Takahashi, Hiromitsu

AU - Dotani, Tadayasu

AU - Kubo, Hidetoshi

AU - Yatsu, Yoichi

AU - Tokanai, Fuyuku

AU - Nakamori, Takeshi

AU - Shibata, Shinpei

AU - Hayato, Asami

AU - Furuzawa, Akihiro

AU - Kishimoto, Yuji

AU - Kitamoto, Shunji

AU - Toma, Kenji

AU - Sadamoto, Masaaki

AU - Yoshinaga, Keigo

AU - Kim, Juyong

AU - Ide, Shunichiro

AU - Kamitsukasa, Fumiyoshi

AU - Anabuki, Naohisa

AU - Tsunemi, Hiroshi

AU - Katagiri, Jun

AU - Sugimoto, Juri

PY - 2014

Y1 - 2014

N2 - 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 hard X-ray (10-80 keV) polarimetry of sources brighter than 10 mCrab. For this purpose, PolariS employs three hard X-ray telescopes and scattering type imaging polarimeters. PolariS 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 (GRBs). Wide field polarimeters based on similar concept as that used in the IKAROS/GAP but with higher sensitivity will be used, and polarization measurement of 10 GRBs per year is expected.

AB - 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 hard X-ray (10-80 keV) polarimetry of sources brighter than 10 mCrab. For this purpose, PolariS employs three hard X-ray telescopes and scattering type imaging polarimeters. PolariS 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 (GRBs). Wide field polarimeters based on similar concept as that used in the IKAROS/GAP but with higher sensitivity will be used, and polarization measurement of 10 GRBs per year is expected.

KW - GRB

KW - Hard X-ray

KW - PolariS

KW - Small Satellite

KW - X-ray Polarimetry

KW - X-ray Scattering

UR - https://www.scopus.com/pages/publications/84922571478

UR - https://www.scopus.com/pages/publications/84922571478#tab=citedBy

U2 - 10.1117/12.2056685

DO - 10.1117/12.2056685

M3 - Conference contribution

AN - SCOPUS:84922571478

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2014

A2 - Takahashi, Tadayuki

A2 - den Herder, Jan-Willem A.

A2 - Bautz, Mark

PB - SPIE

T2 - Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray

Y2 - 22 June 2014 through 26 June 2014

ER -

X-ray γ-ray polarimetry small satellite PolariS

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All Science Journal Classification (ASJC) codes

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