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

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Citations (Scopus)

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.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2014
Subtitle of host publication	Ultraviolet to Gamma Ray
Editors	Tadayuki Takahashi, Jan-Willem A. den Herder, Mark Bautz
Publisher	SPIE
ISBN (Electronic)	9780819496126
DOIs	https://doi.org/10.1117/12.2056685
Publication status	Published - 2014
Externally published	Yes
Event	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray - Montreal, Canada Duration: 22-06-2014 → 26-06-2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9144
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Country/Territory	Canada
City	Montreal
Period	22-06-14 → 26-06-14

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2056685

Cite this

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 Article 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.",

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",

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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, Canada, 22-06-14. https://doi.org/10.1117/12.2056685

X-ray γ-ray polarimetry small satellite PolariS. / Hayashida, Kiyoshi; Yonetoku, Daisuke; Gunji, Shuichi et al.
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).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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.

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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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