Diffuse Gamma-ray Foregrounds
Diffuse Gamma-Ray Foregrounds is a class of astrophysical emission components in gamma-ray astronomy that originate from interstellar processes within the Milky Way, distinguished from extragalactic background signals by their spatial correlation with galactic matter and cosmic-ray interactions.
29
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1.7K
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369
Authors
130
Institutions
Publications per year
2017–2026
5
Parents
29
Clusters of galaxies and the diffuse gamma-ray background
Astroparticle Physics · 1998 · 152 citations · Full text
Natural Sciences, Astronomy, Physics +12
The nature of the Diffuse Gamma-Ray Background
Mattia Fornasa, M. Sánchez‐Conde · Physics Reports · 2015 · 134 citations · Full text
Natural Sciences, Astronomy, Physics +10
CLUSTERS OF GALAXIES AND THE DIFFUSE GAMMA RAY BACKGROUND
S. Colafrancesco, Pasquale Blasi · 1998 · 97 citations
Natural Sciences, Astronomy, Physics +12
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130

Centre National de la Recherche Scientifique
Paris, France
4 h-index
28 publications
12.8K citations

Fermi National Accelerator Laboratory
Batavia, United States
4 h-index
141 publications
2.4K citations
Goddard Space Flight Center
Greenbelt, United States
3 h-index
13 publications
4.8K citations
The University of Tokyo
Tokyo, Japan
3 h-index
11 publications
276 citations

Aarhus University
Aarhus, Denmark
2 h-index
5 publications
177 citations
University of California, Santa Cruz
Santa Cruz, United States
2 h-index
8 publications
3.7K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
2 h-index
3 publications
1.1K citations

Stockholm University
Stockholm, Sweden
2 h-index
4 publications
1.7K citations
1–8 of 130
PRD · 3 publications · 153 citations
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3 publications · 63 citations
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JCAP · 3 publications · 212 citations
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2 publications · 54 citations
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2 publications · 33 citations
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