Calibration and performance studies of the balloon-borne hard X-ray polarimeter PoGO

被引:15
作者
Chauvin, M. [1 ,2 ]
Friis, M. [1 ,2 ]
Jackson, M. [1 ,4 ]
Kawano, T. [3 ]
Kiss, M. [1 ,2 ]
Mikhalev, V. [1 ,2 ]
Ohashi, N. [3 ]
Stana, T. [1 ]
Takahashi, H. [3 ]
Pearce, M. [1 ,2 ]
机构
[1] KTH Royal Inst Technol, Dept Phys, S-10691 Stockholm, Sweden
[2] AlbaNova Univ Ctr, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden
[3] Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan
[4] Cardiff Univ, Phys & Astron, Cardiff CF24 3AA, Wales
基金
瑞典研究理事会;
关键词
X-ray; Polarisation; Compton scattering; Scientific ballooning; Crab; Cygnus X-1; Monte Carlo simulations; CYGNUS X-1; POLARIZATION MEASUREMENTS; CRAB-NEBULA; EMISSION; PATHFINDER; ASTRONOMY; DETECTOR;
D O I
10.1016/j.nima.2017.03.027
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
Polarimetric observations of celestial sources in the hard X-ray band stand to provide new information on emission mechanisms and source geometries. PoGO+ is a Compton scattering polarimeter (20-150 keV) optimised for the observation of the Crab (pulsar and wind nebula) and Cygnus X-1 (black hole binary), from a stratospheric balloon-borne platform launched from the Esrange Space Centre in summer 2016. Prior to flight, the response of the polarimeter has been studied with polarised and unpolarised X-rays allowing a Geant4-based simulation model to be validated. The expected modulation factor for Crab observations is found to be M-Crab = (41.75 +/- 0.85)%, resulting in an expected Minimum Detectable Polarisation (MDP) of 7.3% for a 7 day flight. This will allow a measurement of the Crab polarisation parameters with at least 5 sigma statistical significance assuming a polarisation fraction similar to 20% - a significant improvement over the PoGOLite Pathfinder mission which flew in 2013 and from which the PoGO+ design is developed.
引用
收藏
页码:125 / 133
页数:9
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