X-ray Background Modeling
X-Ray Background Modeling is a scientific method that characterizes the diffuse X-ray emission originating from cosmic sources and instrumental backgrounds by distinguishing astrophysical signals from contaminating components through statistical and physical modeling techniques.
291
Publications
19.6K
Citations
774
Authors
322
Institutions
Publications per year
2017–2026
41
Parents
291
Yoshihiro Ueda, Masayuki Akiyama, G. Hasinger et al. · The Astrophysical Journal · 2014 · 666 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 291
774
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10
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10
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8
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7
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1–5 of 774
322
Institute of Astronomy
Moscow, Russia
20 h-index
53 publications
4.3K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
20 h-index
45 publications
3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
19 h-index
62 publications
5.8K citations
Goddard Space Flight Center
Greenbelt, United States
18 h-index
56 publications
3K citations
National Institute for Astrophysics
Rome, Italy
17 h-index
80 publications
5K citations
Osservatorio astronomico di Bologna
Bologna, Italy
14 h-index
43 publications
3.4K citations

University of Bologna
Bologna, Italy
13 h-index
26 publications
1K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
15 publications
1.1K citations
1–8 of 322
ApJ · 82 publications · 6.2K citations
41
h-index
56 publications · 3.6K citations
33
h-index
24 publications · 2.3K citations
18
h-index
7 publications · 185 citations
7
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5 publications · 850 citations
5
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1–5