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Proceedings Paper

A high-energy Compton polarimeter for the POET SMEX mission
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Paper Abstract

The primary science goal of the Polarimeters for Energetic Transients (POET) mission is to measure the polarization of gamma-ray bursts over a wide energy range, from X rays to soft gamma rays. The higher-energy portion of this band (50 - 500 keV) will be covered by the High Energy Polarimeter (HEP) instrument, a non-imaging, wide field of view Compton polarimeter. Incident high-energy photons will Compton scatter in low-Z, plastic scintillator detector elements and be subsequently absorbed in high-Z, CsI(Tl) scintillator elements; polarization is detected by measuring an asymmetry in the azimuthal scatter angle distribution. The HEP design is based on our considerable experience with the development and flight of the Gamma-Ray Polarimeter Experiment (GRAPE) balloon payload. We present the design of the POET HEP instrument, which incorporates lessons learned from the GRAPE balloon design and previous work on Explorer proposal efforts, and its expected performance on a two-year SMEX mission.

Paper Details

Date Published: 24 July 2014
PDF: 6 pages
Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91441I (24 July 2014); doi: 10.1117/12.2056868
Show Author Affiliations
Peter F. Bloser, Space Science Ctr., The Univ. of New Hampshire (United States)
Mark L. McConnell, Space Science Ctr., The Univ. of New Hampshire (United States)
Jason S. Legere, Space Science Ctr., The Univ. of New Hampshire (United States)
Camden D. Ertley, Space Science Ctr., The Univ. of New Hampshire (United States)
Joanne E. Hill, NASA Goddard Space Flight Ctr. (United States)
Marc Kippen, Los Alamos National Lab. (United States)
James M. Ryan, Space Science Ctr., The Univ. of New Hampshire (United States)


Published in SPIE Proceedings Vol. 9144:
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz, Editor(s)

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