High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite

T. Mizuno; M. Arimoto; M. Axelsson; C. I. Björnsson; G. Bogaert; P. Carlson; W. Craig; Y. Fukazawa; S. Gunji; L. Hjalmarsdotter; T. Kamae; Y. Kanai; J. Kataoka; J. Katsuta; N. Kawai; M. Kiss; W. Klamra; S. Larsson; G. Madejski; C. Marini Bettolo; J. Ng; M. Pearce; F. Ryde; H. Tajima; H. Takahash; T. Takahashi; T. Tanaka; T. Thurston; M. Ueno; G. Varner; H. Yoshida

doi:10.1109/NSSMIC.2007.4436669

High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite

T. Mizuno^*, M. Arimoto, M. Axelsson, C. I. Björnsson, G. Bogaert, P. Carlson, W. Craig, Y. Fukazawa, S. Gunji, L. Hjalmarsdotter, T. Kamae, Y. Kanai, J. Kataoka, J. Katsuta, N. Kawai, M. Kiss, W. Klamra, S. Larsson, G. Madejski, C. Marini BettoloJ. Ng, M. Pearce, F. Ryde, H. Tajima, H. Takahash, T. Takahashi, T. Tanaka, T. Thurston, M. Ueno, G. Varner, H. Yoshida

^*Corresponding author for this work

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

1 Citation (Scopus)

Abstract

The Polarized Gamma-ray Observer - Lightweight Version (PoGOLite) is a new balloon experiment capable of detecting 10% polarization from a 200 mCrab source in the 25-80 keV energy range in a single 6-hour flight for the first time. Polarization measurements of hard X-rays and soft gamma-rays are expected to provide a powerful probe into high-energy emission mechanisms as well as source geometries. PoGOLite uses Compton scattering and photo-absorption to measure polarization in an array of 217 well-type phoswich detector cells made of plastic and BGO scintillators. The adoption of a well-type phoswich counter concept and a thick polyethylene neutron shield provides a narrow field-of-view (1.25 msr), a large effective area (≥ 250 cm² at 40-50 keV), a high modulation factor (more than 25 %) and the low background (∼100 mCrab) required to conduct high-sensitivity polarization measurements. Through tests in laboratories and accelerator facilities of a scaled-down prototype with the front-end electronics of flight design and an extensive study by Monte-Carlo simulation, we have demonstrated high instrument performance. PoGOLite will be ready for a first engineering flight in 2009 and a science flight in 2010, during which polarization signals from the Crab Nebula/pulsar, Cygnus X-1 and other objects will be observed.

Original language	English
Title of host publication	2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC
Pages	2538-2544
Number of pages	7
DOIs	https://doi.org/10.1109/NSSMIC.2007.4436669
Publication status	Published - 2007
Externally published	Yes
Event	2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC - Honolulu, HI, United States Duration: 2007 Oct 27 → 2007 Nov 3

Publication series

Name	IEEE Nuclear Science Symposium Conference Record
Volume	4
ISSN (Print)	1095-7863

Conference

Conference	2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC
Country/Territory	United States
City	Honolulu, HI
Period	07/10/27 → 07/11/3

ASJC Scopus subject areas

Radiation
Nuclear and High Energy Physics
Radiology Nuclear Medicine and imaging

Access to Document

10.1109/NSSMIC.2007.4436669

Cite this

Mizuno, T., Arimoto, M., Axelsson, M., Björnsson, C. I., Bogaert, G., Carlson, P., Craig, W., Fukazawa, Y., Gunji, S., Hjalmarsdotter, L., Kamae, T., Kanai, Y., Kataoka, J., Katsuta, J., Kawai, N., Kiss, M., Klamra, W., Larsson, S., Madejski, G., ... Yoshida, H. (2007). High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite. In 2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC (pp. 2538-2544). [4436669] (IEEE Nuclear Science Symposium Conference Record; Vol. 4). https://doi.org/10.1109/NSSMIC.2007.4436669

High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite. / Mizuno, T.; Arimoto, M.; Axelsson, M. et al.

2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC. 2007. p. 2538-2544 4436669 (IEEE Nuclear Science Symposium Conference Record; Vol. 4).

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

Mizuno, T, Arimoto, M, Axelsson, M, Björnsson, CI, Bogaert, G, Carlson, P, Craig, W, Fukazawa, Y, Gunji, S, Hjalmarsdotter, L, Kamae, T, Kanai, Y, Kataoka, J, Katsuta, J, Kawai, N, Kiss, M, Klamra, W, Larsson, S, Madejski, G, Bettolo, CM, Ng, J, Pearce, M, Ryde, F, Tajima, H, Takahash, H, Takahashi, T, Tanaka, T, Thurston, T, Ueno, M, Varner, G & Yoshida, H 2007, High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite. in 2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC., 4436669, IEEE Nuclear Science Symposium Conference Record, vol. 4, pp. 2538-2544, 2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC, Honolulu, HI, United States, 07/10/27. https://doi.org/10.1109/NSSMIC.2007.4436669

@inproceedings{8e4bc1ebfd11454b965e841edcd953a2,

title = "High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite",

abstract = "The Polarized Gamma-ray Observer - Lightweight Version (PoGOLite) is a new balloon experiment capable of detecting 10% polarization from a 200 mCrab source in the 25-80 keV energy range in a single 6-hour flight for the first time. Polarization measurements of hard X-rays and soft gamma-rays are expected to provide a powerful probe into high-energy emission mechanisms as well as source geometries. PoGOLite uses Compton scattering and photo-absorption to measure polarization in an array of 217 well-type phoswich detector cells made of plastic and BGO scintillators. The adoption of a well-type phoswich counter concept and a thick polyethylene neutron shield provides a narrow field-of-view (1.25 msr), a large effective area (≥ 250 cm2 at 40-50 keV), a high modulation factor (more than 25 %) and the low background (∼100 mCrab) required to conduct high-sensitivity polarization measurements. Through tests in laboratories and accelerator facilities of a scaled-down prototype with the front-end electronics of flight design and an extensive study by Monte-Carlo simulation, we have demonstrated high instrument performance. PoGOLite will be ready for a first engineering flight in 2009 and a science flight in 2010, during which polarization signals from the Crab Nebula/pulsar, Cygnus X-1 and other objects will be observed.",

author = "T. Mizuno and M. Arimoto and M. Axelsson and Bj{\"o}rnsson, {C. I.} and G. Bogaert and P. Carlson and W. Craig and Y. Fukazawa and S. Gunji and L. Hjalmarsdotter and T. Kamae and Y. Kanai and J. Kataoka and J. Katsuta and N. Kawai and M. Kiss and W. Klamra and S. Larsson and G. Madejski and Bettolo, {C. Marini} and J. Ng and M. Pearce and F. Ryde and H. Tajima and H. Takahash and T. Takahashi and T. Tanaka and T. Thurston and M. Ueno and G. Varner and H. Yoshida",

year = "2007",

doi = "10.1109/NSSMIC.2007.4436669",

language = "English",

isbn = "1424409233",

series = "IEEE Nuclear Science Symposium Conference Record",

pages = "2538--2544",

booktitle = "2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC",

note = "2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC ; Conference date: 27-10-2007 Through 03-11-2007",

}

TY - GEN

T1 - High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite

AU - Mizuno, T.

AU - Arimoto, M.

AU - Axelsson, M.

AU - Björnsson, C. I.

AU - Bogaert, G.

AU - Carlson, P.

AU - Craig, W.

AU - Fukazawa, Y.

AU - Gunji, S.

AU - Hjalmarsdotter, L.

AU - Kamae, T.

AU - Kanai, Y.

AU - Kataoka, J.

AU - Katsuta, J.

AU - Kawai, N.

AU - Kiss, M.

AU - Klamra, W.

AU - Larsson, S.

AU - Madejski, G.

AU - Bettolo, C. Marini

AU - Ng, J.

AU - Pearce, M.

AU - Ryde, F.

AU - Tajima, H.

AU - Takahash, H.

AU - Takahashi, T.

AU - Tanaka, T.

AU - Thurston, T.

AU - Ueno, M.

AU - Varner, G.

AU - Yoshida, H.

PY - 2007

Y1 - 2007

N2 - The Polarized Gamma-ray Observer - Lightweight Version (PoGOLite) is a new balloon experiment capable of detecting 10% polarization from a 200 mCrab source in the 25-80 keV energy range in a single 6-hour flight for the first time. Polarization measurements of hard X-rays and soft gamma-rays are expected to provide a powerful probe into high-energy emission mechanisms as well as source geometries. PoGOLite uses Compton scattering and photo-absorption to measure polarization in an array of 217 well-type phoswich detector cells made of plastic and BGO scintillators. The adoption of a well-type phoswich counter concept and a thick polyethylene neutron shield provides a narrow field-of-view (1.25 msr), a large effective area (≥ 250 cm2 at 40-50 keV), a high modulation factor (more than 25 %) and the low background (∼100 mCrab) required to conduct high-sensitivity polarization measurements. Through tests in laboratories and accelerator facilities of a scaled-down prototype with the front-end electronics of flight design and an extensive study by Monte-Carlo simulation, we have demonstrated high instrument performance. PoGOLite will be ready for a first engineering flight in 2009 and a science flight in 2010, during which polarization signals from the Crab Nebula/pulsar, Cygnus X-1 and other objects will be observed.

AB - The Polarized Gamma-ray Observer - Lightweight Version (PoGOLite) is a new balloon experiment capable of detecting 10% polarization from a 200 mCrab source in the 25-80 keV energy range in a single 6-hour flight for the first time. Polarization measurements of hard X-rays and soft gamma-rays are expected to provide a powerful probe into high-energy emission mechanisms as well as source geometries. PoGOLite uses Compton scattering and photo-absorption to measure polarization in an array of 217 well-type phoswich detector cells made of plastic and BGO scintillators. The adoption of a well-type phoswich counter concept and a thick polyethylene neutron shield provides a narrow field-of-view (1.25 msr), a large effective area (≥ 250 cm2 at 40-50 keV), a high modulation factor (more than 25 %) and the low background (∼100 mCrab) required to conduct high-sensitivity polarization measurements. Through tests in laboratories and accelerator facilities of a scaled-down prototype with the front-end electronics of flight design and an extensive study by Monte-Carlo simulation, we have demonstrated high instrument performance. PoGOLite will be ready for a first engineering flight in 2009 and a science flight in 2010, during which polarization signals from the Crab Nebula/pulsar, Cygnus X-1 and other objects will be observed.

UR - http://www.scopus.com/inward/record.url?scp=48149109282&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=48149109282&partnerID=8YFLogxK

U2 - 10.1109/NSSMIC.2007.4436669

DO - 10.1109/NSSMIC.2007.4436669

M3 - Conference contribution

AN - SCOPUS:48149109282

SN - 1424409233

SN - 9781424409235

T3 - IEEE Nuclear Science Symposium Conference Record

SP - 2538

EP - 2544

BT - 2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC

T2 - 2007 IEEE Nuclear Science Symposium and Medical Imaging Conference, NSS-MIC

Y2 - 27 October 2007 through 3 November 2007

ER -

High sensitivity balloon-borne hard X-ray/soft Gamma-ray polarimeter PoGOLite

Abstract

Publication series

Conference

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this