Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite

M. Arimoto; Y. Kanai; M. Ueno; J. Kataoka; N. Kawai; T. Tanaka; K. Yamamoto; H. Takahashi; T. Mizuno; Y. Fukazawa; M. Axelsson; M. Kiss; C. Marini Bettolo; P. Carlson; W. Klamra; M. Pearce; P. Chen; B. Craig; T. Kamae; G. Madejski; J. S.T. Ng; R. Rogers; H. Tajima; T. S. Thurston; Y. Saito; T. Takahashi; S. Gunji; C. I. Bjornsson; S. Larsson; F. Ryde; G. Bogaert; G. Varner

doi:10.1016/j.physe.2007.06.051

Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite

M. Arimoto^*, Y. Kanai, M. Ueno, J. Kataoka, N. Kawai, T. Tanaka, K. Yamamoto, H. Takahashi, T. Mizuno, Y. Fukazawa, M. Axelsson, M. Kiss, C. Marini Bettolo, P. Carlson, W. Klamra, M. Pearce, P. Chen, B. Craig, T. Kamae, G. MadejskiJ. S.T. Ng, R. Rogers, H. Tajima, T. S. Thurston, Y. Saito, T. Takahashi, S. Gunji, C. I. Bjornsson, S. Larsson, F. Ryde, G. Bogaert, G. Varner

^*この研究の対応する著者

研究成果: Article › 査読

抄録

Measurements of polarization play a crucial role in the understanding of the dominant emission mechanism of astronomical sources. Polarized Gamma-ray Observer-Light version (PoGOLite) is a balloon-borne astronomical soft gamma-ray polarimeter at the 25-80 keV band. The PoGOLite detector consists of a hexagonal close-packed array of 217 Phoswich detector cells (PDCs) and side anti-coincidence shields (SASs) made of BGO crystals surrounding PDCs. Each PDC consists of a slow hollow scintillator, a fast scintillator and a BGO crystal that connects to a photomultiplier tube at the end. To examine the PoGOLite's capability and estimate the performance, we conducted experiments with the PDC using radioisotope ²⁴¹Am. In addition, we compared this result with performance expected by Monte Carlo simulation with Geant4. As a result, we found that the actual PDC has the capability to detect a 100 m Crab source until 80 keV.

本文言語	English
ページ（範囲）	438-441
ページ数	4
ジャーナル	Physica E: Low-Dimensional Systems and Nanostructures
巻	40
号	2
DOI	https://doi.org/10.1016/j.physe.2007.06.051
出版ステータス	Published - 2007 12月
外部発表	はい

ASJC Scopus subject areas

電子材料、光学材料、および磁性材料
原子分子物理学および光学
凝縮系物理学

文献へのアクセス

10.1016/j.physe.2007.06.051

他のファイルとリンク

引用スタイル

Arimoto, M., Kanai, Y., Ueno, M., Kataoka, J., Kawai, N., Tanaka, T., Yamamoto, K., Takahashi, H., Mizuno, T., Fukazawa, Y., Axelsson, M., Kiss, M., Marini Bettolo, C., Carlson, P., Klamra, W., Pearce, M., Chen, P., Craig, B., Kamae, T., ... Varner, G. (2007). Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite. Physica E: Low-Dimensional Systems and Nanostructures, 40(2), 438-441. https://doi.org/10.1016/j.physe.2007.06.051

Arimoto, M, Kanai, Y, Ueno, M, Kataoka, J, Kawai, N, Tanaka, T, Yamamoto, K, Takahashi, H, Mizuno, T, Fukazawa, Y, Axelsson, M, Kiss, M, Marini Bettolo, C, Carlson, P, Klamra, W, Pearce, M, Chen, P, Craig, B, Kamae, T, Madejski, G, Ng, JST, Rogers, R, Tajima, H, Thurston, TS, Saito, Y, Takahashi, T, Gunji, S, Bjornsson, CI, Larsson, S, Ryde, F, Bogaert, G & Varner, G 2007, 'Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite', Physica E: Low-Dimensional Systems and Nanostructures, vol. 40, no. 2, pp. 438-441. https://doi.org/10.1016/j.physe.2007.06.051

@article{94df7c61c90b4381a0abb520025ac1d6,

title = "Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite",

abstract = "Measurements of polarization play a crucial role in the understanding of the dominant emission mechanism of astronomical sources. Polarized Gamma-ray Observer-Light version (PoGOLite) is a balloon-borne astronomical soft gamma-ray polarimeter at the 25-80 keV band. The PoGOLite detector consists of a hexagonal close-packed array of 217 Phoswich detector cells (PDCs) and side anti-coincidence shields (SASs) made of BGO crystals surrounding PDCs. Each PDC consists of a slow hollow scintillator, a fast scintillator and a BGO crystal that connects to a photomultiplier tube at the end. To examine the PoGOLite's capability and estimate the performance, we conducted experiments with the PDC using radioisotope 241Am. In addition, we compared this result with performance expected by Monte Carlo simulation with Geant4. As a result, we found that the actual PDC has the capability to detect a 100 m Crab source until 80 keV.",

keywords = "Balloon experiment, Gamma-ray, Polarization, X-ray",

author = "M. Arimoto and Y. Kanai and M. Ueno and J. Kataoka and N. Kawai and T. Tanaka and K. Yamamoto and H. Takahashi and T. Mizuno and Y. Fukazawa and M. Axelsson and M. Kiss and {Marini Bettolo}, C. and P. Carlson and W. Klamra and M. Pearce and P. Chen and B. Craig and T. Kamae and G. Madejski and Ng, {J. S.T.} and R. Rogers and H. Tajima and Thurston, {T. S.} and Y. Saito and T. Takahashi and S. Gunji and Bjornsson, {C. I.} and S. Larsson and F. Ryde and G. Bogaert and G. Varner",

note = "Funding Information: This work is supported by Grant-in-Aid for Science Research (KAKENHI) 16340055, Japan Society for the Promotion of Science (JSPS); by Kavli Institute for Particle Astrophysics and Cosmology, Stanford University; and by Knut and Alice Wallenberg Foundation and The Swedish National Space Board; M.A. is supported by a 21st Century COE Program at TokyoTech “Nanometer-Scale Quantum Physics” by the Ministry of Education, Culture, Sports, Science and Technology.",

year = "2007",

month = dec,

doi = "10.1016/j.physe.2007.06.051",

language = "English",

volume = "40",

pages = "438--441",

journal = "Physica E: Low-Dimensional Systems and Nanostructures",

issn = "1386-9477",

publisher = "Elsevier",

number = "2",

}

TY - JOUR

T1 - Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite

AU - Arimoto, M.

AU - Kanai, Y.

AU - Ueno, M.

AU - Kataoka, J.

AU - Kawai, N.

AU - Tanaka, T.

AU - Yamamoto, K.

AU - Takahashi, H.

AU - Mizuno, T.

AU - Fukazawa, Y.

AU - Axelsson, M.

AU - Kiss, M.

AU - Marini Bettolo, C.

AU - Carlson, P.

AU - Klamra, W.

AU - Pearce, M.

AU - Chen, P.

AU - Craig, B.

AU - Kamae, T.

AU - Madejski, G.

AU - Ng, J. S.T.

AU - Rogers, R.

AU - Tajima, H.

AU - Thurston, T. S.

AU - Saito, Y.

AU - Takahashi, T.

AU - Gunji, S.

AU - Bjornsson, C. I.

AU - Larsson, S.

AU - Ryde, F.

AU - Bogaert, G.

AU - Varner, G.

N1 - Funding Information: This work is supported by Grant-in-Aid for Science Research (KAKENHI) 16340055, Japan Society for the Promotion of Science (JSPS); by Kavli Institute for Particle Astrophysics and Cosmology, Stanford University; and by Knut and Alice Wallenberg Foundation and The Swedish National Space Board; M.A. is supported by a 21st Century COE Program at TokyoTech “Nanometer-Scale Quantum Physics” by the Ministry of Education, Culture, Sports, Science and Technology.

PY - 2007/12

Y1 - 2007/12

N2 - Measurements of polarization play a crucial role in the understanding of the dominant emission mechanism of astronomical sources. Polarized Gamma-ray Observer-Light version (PoGOLite) is a balloon-borne astronomical soft gamma-ray polarimeter at the 25-80 keV band. The PoGOLite detector consists of a hexagonal close-packed array of 217 Phoswich detector cells (PDCs) and side anti-coincidence shields (SASs) made of BGO crystals surrounding PDCs. Each PDC consists of a slow hollow scintillator, a fast scintillator and a BGO crystal that connects to a photomultiplier tube at the end. To examine the PoGOLite's capability and estimate the performance, we conducted experiments with the PDC using radioisotope 241Am. In addition, we compared this result with performance expected by Monte Carlo simulation with Geant4. As a result, we found that the actual PDC has the capability to detect a 100 m Crab source until 80 keV.

AB - Measurements of polarization play a crucial role in the understanding of the dominant emission mechanism of astronomical sources. Polarized Gamma-ray Observer-Light version (PoGOLite) is a balloon-borne astronomical soft gamma-ray polarimeter at the 25-80 keV band. The PoGOLite detector consists of a hexagonal close-packed array of 217 Phoswich detector cells (PDCs) and side anti-coincidence shields (SASs) made of BGO crystals surrounding PDCs. Each PDC consists of a slow hollow scintillator, a fast scintillator and a BGO crystal that connects to a photomultiplier tube at the end. To examine the PoGOLite's capability and estimate the performance, we conducted experiments with the PDC using radioisotope 241Am. In addition, we compared this result with performance expected by Monte Carlo simulation with Geant4. As a result, we found that the actual PDC has the capability to detect a 100 m Crab source until 80 keV.

KW - Balloon experiment

KW - Gamma-ray

KW - Polarization

KW - X-ray

UR - http://www.scopus.com/inward/record.url?scp=36049025220&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=36049025220&partnerID=8YFLogxK

U2 - 10.1016/j.physe.2007.06.051

DO - 10.1016/j.physe.2007.06.051

M3 - Article

AN - SCOPUS:36049025220

VL - 40

SP - 438

EP - 441

JO - Physica E: Low-Dimensional Systems and Nanostructures

JF - Physica E: Low-Dimensional Systems and Nanostructures

SN - 1386-9477

IS - 2

ER -

Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite

抄録

ASJC Scopus subject areas

文献へのアクセス

他のファイルとリンク

フィンガープリント

引用スタイル