Linear Polarimetry with γ→e+e− Conversions
LLR, Ecole polytechnique & CNRS/IN2P3, 91128 Palaiseau, France
Academic Editors: Emmanouil Angelakis, Markus Boettcher and Jose L. Gómez
Galaxies 2017, 5(4), 72; https://doi.org/10.3390/galaxies5040072
Received: 25 September 2017 / Revised: 22 October 2017 / Accepted: 25 October 2017 / Published: 1 November 2017
(This article belongs to the Special Issue Polarised Emission from Astrophysical Jets)
Keywords:
gamma-ray astronomy; gamma-ray polarimetry; pair conversion; time projection chamber; gas detector; optimal methods; Kalman filter; Bayesian method
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This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
MDPI and ACS Style
Bernard, D. Linear Polarimetry with γ→e+e− Conversions. Galaxies 2017, 5, 72. https://doi.org/10.3390/galaxies5040072
AMA Style
Bernard D. Linear Polarimetry with γ→e+e− Conversions. Galaxies. 2017; 5(4):72. https://doi.org/10.3390/galaxies5040072
Chicago/Turabian StyleBernard, Denis. 2017. "Linear Polarimetry with γ→e+e− Conversions" Galaxies 5, no. 4: 72. https://doi.org/10.3390/galaxies5040072
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