29 July 2014 POET: a SMEX mission for gamma ray burst polarimetry
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Polarimeters for Energetic Transients (POET) is a mission concept designed to t within the envelope of a NASA Small Explorer (SMEX) mission. POET will use X-ray and gamma-ray polarimetry to uncover the energy release mechanism associated with the formation of stellar-mass black holes and investigate the physics of extreme magnetic ields in the vicinity of compact objects. Two wide-FoV, non-imaging polarimeters will provide polarization measurements over the broad energy range from about 2 keV up to about 500 keV. A Compton scatter polarimeter, using an array of independent scintillation detector elements, will be used to collect data from 50 keV up to 500 keV. At low energies (2{15 keV), data will be provided by a photoelectric polarimeter based on the use of a Time Projection Chamber for photoelectron tracking. During a two-year baseline mission, POET will be able to collect data that will allow us to distinguish between three basic models for the inner jet of gamma-ray bursts.
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Mark L. McConnell, Mark L. McConnell, Matthew Baring, Matthew Baring, Peter Bloser, Peter Bloser, Joseph F. Dwyer, Joseph F. Dwyer, A. Gordon Emslie, A. Gordon Emslie, Camden D. Ertley, Camden D. Ertley, Jochen Greiner, Jochen Greiner, Alice K. Harding, Alice K. Harding, Dieter H. Hartmann, Dieter H. Hartmann, Joanne E. Hill, Joanne E. Hill, Philip Kaaret, Philip Kaaret, R. Marc Kippen, R. Marc Kippen, David Mattingly, David Mattingly, Sheila McBreen, Sheila McBreen, Mark Pearce, Mark Pearce, Nicolas Produit, Nicolas Produit, James M. Ryan, James M. Ryan, Felix Ryde, Felix Ryde, Takanori Sakamoto, Takanori Sakamoto, Kenji Toma, Kenji Toma, W. Thomas Vestrand, W. Thomas Vestrand, Bing Zhang, Bing Zhang, } "POET: a SMEX mission for gamma ray burst polarimetry", Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91440O (29 July 2014); doi: 10.1117/12.2056905; https://doi.org/10.1117/12.2056905

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