24 July 2014 Monte-Carlo estimation of the inflight performance of the GEMS satellite x-ray polarimeter
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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, Takao Kitaguchi, Toru Tamagawa, Toru Tamagawa, Asami Hayato, Asami Hayato, Teruaki Enoto, Teruaki Enoto, Akifumi Yoshikawa, Akifumi Yoshikawa, Kenta Kaneko, Kenta Kaneko, Yoko Takeuchi, Yoko Takeuchi, Kevin Black, Kevin Black, Joanne Hill, Joanne Hill, Keith Jahoda, Keith Jahoda, John Krizmanic, John Krizmanic, Steven Sturner, Steven Sturner, Scott Griffiths, Scott Griffiths, Philip Kaaret, Philip Kaaret, Hannah Marlowe, 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); doi: 10.1117/12.2057334; https://doi.org/10.1117/12.2057334


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