Diffuse Extragalactic X-ray Background
The Diffuse Extragalactic X-Ray Background is the isotropic and persistent flux of X-ray photons originating from outside the Milky Way, distinguished from discrete extragalactic sources by its spatially unresolved and all-sky-distributed nature, arising from the superposition of unresolved point sources and potentially truly diffuse processes in the high-energy universe.
189
Publications
10.8K
Citations
527
Authors
224
Institutions
Publications per year
2017–2026
9
Variants
Cosmic X-ray Background
Parents
189
Cosmic X-ray surveys of distant active galaxies
W. N. Brandt, D. M. Alexander · The Astronomy and Astrophysics Review · 2015 · 337 citations · Full text
Natural Sciences, Astronomy, Physics +14
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224
Goddard Space Flight Center
Greenbelt, United States
17 h-index
47 publications
2.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
15 h-index
42 publications
1.8K citations
Institute of Space and Astronautical Science
Tokyo, Japan
13 h-index
37 publications
2.5K citations
Japan Aerospace Exploration Agency
Tokyo, Japan
10 h-index
29 publications
2.2K citations

University of Leicester
Leicester, United Kingdom
10 h-index
29 publications
1.2K citations

Johns Hopkins University
Baltimore, United States
9 h-index
11 publications
710 citations
Osservatorio astronomico di Bologna
Bologna, Italy
8 h-index
9 publications
421 citations
National Institute for Astrophysics
Rome, Italy
8 h-index
17 publications
914 citations
1–8 of 224
ApJ · 80 publications · 5K citations
35
h-index
23 publications · 1.6K citations
17
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18 publications · 990 citations
14
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12 publications · 450 citations
12
h-index
7 publications · 397 citations
7
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