X-ray Reflection
X-Ray Reflection is a theoretical framework in high-energy astrophysics that describes the process by which X-rays emitted from an accreting compact object in a binary system are scattered and reprocessed by surrounding accretion disk material, producing characteristic spectral features such as the Compton hump and iron Kα emission line.
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2017–2026
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Surface Studies of Solids by Total Reflection of X-Rays
L. G. Parratt · Physical Review · 1954 · 5.1K citations
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Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany
29 publications · 3.4K citations
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University of Cambridge
Cambridge, United Kingdom
49 h-index
207 publications
15.3K citations
Goddard Space Flight Center
Greenbelt, United States
43 h-index
218 publications
13.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
40 h-index
140 publications
14.5K citations
California Institute of Technology
Pasadena, United States
40 h-index
188 publications
11K citations
University of Maryland, College Park
College Park, United States
38 h-index
82 publications
9.7K citations
Institute of Astronomy
Moscow, Russia
38 h-index
105 publications
13.9K citations
University of Michigan
Ann Arbor, United States
35 h-index
78 publications
5K citations

Centre National de la Recherche Scientifique
Paris, France
35 h-index
206 publications
8K citations
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ApJ · 154 publications · 12K citations
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190 publications · 15.5K citations
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PRB · 54 publications · 4.2K citations
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60 publications · 2.9K citations
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90 publications · 2.6K citations
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