Author/Authors :
M. Arimoto، نويسنده , , Y. Kanai، نويسنده , , M. Ueno، نويسنده , , J. Kataoka، نويسنده , , N. Kawai، نويسنده , , T. Tanaka، نويسنده , , K. Yamamoto، نويسنده , , H. Takahashi، نويسنده , , T. Mizuno، نويسنده , , Y. Fukazawa، نويسنده , , M. Axelsson، نويسنده , , M. Kiss، نويسنده , , C. Marini Bettolo، نويسنده , , P. Carlson، نويسنده , , W. Klamra، نويسنده , , M. Pearce، نويسنده , , P. Chen، نويسنده , , B. Craig، نويسنده , , T. Kamae، نويسنده , , G. Madejski، نويسنده , , et al.، نويسنده ,
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 PoGOLiteʹs 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 :
Polarization , Balloon experiment , Gamma-ray , X-ray
