Paper
24 July 2014 Monte-Carlo estimation of the inflight performance of the GEMS satellite x-ray polarimeter
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Abstract
We report a Monte-Carlo estimation of the in-orbit performance of a cosmic X-ray polarimeter designed to be installed on the focal plane of a small satellite. The simulation uses GEANT for the transport of photons and energetic particles and results from Magboltz for the transport of secondary electrons in the detector gas. We validated the simulation by comparing spectra and modulation curves with actual data taken with radioactive sources and an X-ray generator. We also estimated the in-orbit background induced by cosmic radiation in low Earth orbit.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Takao Kitaguchi, Toru Tamagawa, Asami Hayato, Teruaki Enoto, Akifumi Yoshikawa, Kenta Kaneko, Yoko Takeuchi, Kevin Black, Joanne Hill, Keith Jahoda, John Krizmanic, Steven Sturner, Scott Griffiths, Philip Kaaret, and Hannah Marlowe "Monte-Carlo estimation of the inflight performance of the GEMS satellite x-ray polarimeter", Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91444L (24 July 2014); https://doi.org/10.1117/12.2057334
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Cited by 5 scholarly publications.
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KEYWORDS
X-rays

Polarimetry

Electrons

Monte Carlo methods

Particles

Modulation

Sensors

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