Galactic Diffuse Gamma-ray Background

Galactic Diffuse Gamma-Ray Background is a component of diffuse gamma-ray emission that originates from widespread cosmic-ray interactions with interstellar matter and radiation fields throughout the Milky Way, distinguished from point sources and extragalactic backgrounds by its smooth spatial distribution and galactic-plane concentration.

285

Publications

21.9K

Citations

1.8K

Authors

435

Institutions

Publications per year

2017–2026

49

Authors

1.8K

  1. AW
    A. W. Strong

    Max Planck Institute for Extraterrestrial Physics, Germany

    20 publications · 6.2K citations

    17

    h-index

  2. IV
    I. V. Moskalenko

    Stanford University, United States

    17 publications · 6.7K citations

    16

    h-index

  3. OR
    O. Reimer

    Centre National de la Recherche Scientifique, France

    16 publications · 7K citations

    14

    h-index

  4. DJ
    D. J. Thompson

    Goddard Space Flight Center, United States

    14 publications · 5.8K citations

    14

    h-index

  5. TA
    T. A. Porter

    Stanford University, United States

    14 publications · 5.3K citations

    13

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 69 publications · 6.8K citations

    35

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 21 publications · 1.6K citations

    19

    h-index

  3. 17

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 15 publications · 901 citations

    15

    h-index

  5. Astronomy and Astrophysics

    18 publications · 937 citations

    15

    h-index

1–5