Using X-Ray Polarimetry to Probe the Physics of Black Holes and Neutron Stars
Date Issued
2019
Author(s)
Krawczynski, Henric
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Ingram, Adam R.
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Taverna, Roberto
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Turolla, Roberto
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Kislat, Fabian
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Cheung, C. C. Teddy
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Sinha, Kuver
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Zhang, Haocheng
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Heyl, Jeremy
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Madejski, Greg
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Kallman, Tim
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Jahoda, Keith M.
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Abarr, Quin
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Baring, Matthew G.
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Baldini, Luca
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Begelman, Mitchell
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Böttcher, Markus
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Cackett, Edward
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Caiazzo, Ilaria
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Coppi, Paolo
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Dexter, Jason
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Fortin, Jean-Francois
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Gammie, Charles
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Gaskin, Jessica A.
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Giannios, Dimitrios
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Ghosh, Pranab
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Harding, Alice K.
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Hartmann, Dieter H.
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Hayashida, Kiyoshi
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Jorstad, Svetlana G.
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Kaaret, Philip
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Kitaguchi, Takao
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Latronico, Luca
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Maccarone, Thomas
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Marscher, Alan
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Marshall, Herman
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McConnell, Mark
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Miller, Jon M.
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O'Dell, Stephen L.
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Özel, Feryal
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Okajima, Takashi
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Pearce, Mark
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Perkins, Jeremy
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Ramsey, Brian D.
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Romani, Roger W.
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Schnittman, Jeremy D.
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Sgro, Carmelo
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Takahashi, Hiromitsu
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Tamagawa, Toru
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Tomsick, John
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Weisskopf, Martin C.
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Younes, George
Abstract
This white paper highlights compact object and fundamental physics science opportunities afforded by high-throughput broadband (0.1-60 keV) X-ray polarization observations. The polarimetric observations can reveal the inner workings of high-energy sources, and allow us to test physical laws in the extreme conditions close to compact objects.
Volume
51
Issue
3
Start page
150
Issn Identifier
2330-9458
Ads BibCode
2019BAAS...51c.150K
Rights
open.access
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21598543805290.pdf
Description
postprint
Size
1.13 MB
Format
Adobe PDF
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