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

Authors :
Mizuno, T.
Arimoto, M.
Axelsson, Magnus
Björnsson, C. -I
Bogaert, G.
Carlson, Per
Craig, W.
Fukazawa, Y.
Gunji, S.
Hjalmarsdotter, L.
Kamae, T.
Kanai, Y.
Kataoka, J.
Katsuta, J.
Kawai, N.
Kiss, Mózsi Bank
Klamra, Wlodzimierz
Larsson, S.
Madejski, G.
Bettolo, Cecilia M.
Ng, J.
Pearce, Mark
Ryde, Felix
Tajima, H.
Takahash, H.
Takahashi, T.
Tanaka, T.
Thurston, T.
Ueno, M.
Varner, G.
Yoshida, H.
Mizuno, T.
Arimoto, M.
Axelsson, Magnus
Björnsson, C. -I
Bogaert, G.
Carlson, Per
Craig, W.
Fukazawa, Y.
Gunji, S.
Hjalmarsdotter, L.
Kamae, T.
Kanai, Y.
Kataoka, J.
Katsuta, J.
Kawai, N.
Kiss, Mózsi Bank
Klamra, Wlodzimierz
Larsson, S.
Madejski, G.
Bettolo, Cecilia M.
Ng, J.
Pearce, Mark
Ryde, Felix
Tajima, H.
Takahash, H.
Takahashi, T.
Tanaka, T.
Thurston, T.
Ueno, M.
Varner, G.
Yoshida, H.
Publication Year :
2007

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 ( gt; 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.<br />QC 20120301

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1234625175
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1109.NSSMIC.2007.4436669