Galactic Diffuse Emission Modeling

Galactic Diffuse Emission Modeling is a computational and theoretical framework in high-energy astrophysics that characterizes the spatial, spectral, and temporal distribution of gamma-ray photons originating from interstellar processes within the Milky Way, distinguishing it from analyses focused on point sources or extragalactic emission.

153

Publications

19.4K

Citations

1.4K

Authors

419

Institutions

Publications per year

2017–2026

35

Authors

1.4K

  1. AW
    A. W. Strong

    Max Planck Institute for Extraterrestrial Physics, Germany

    14 publications · 5.7K citations

    13

    h-index

  2. IV
    I. V. Moskalenko

    Stanford University, United States

    13 publications · 6.2K citations

    13

    h-index

  3. OR
    O. Reimer

    Centre National de la Recherche Scientifique, France

    12 publications · 5.9K citations

    11

    h-index

  4. TA
    T. A. Porter

    Stanford University, United States

    9 publications · 4.1K citations

    9

    h-index

  5. GJ
    G. Jóhannesson

    Stanford University, United States

    9 publications · 4.6K citations

    9

    h-index

1–5 of 1.4K

Venues

  1. The Astrophysical Journal

    ApJ · 46 publications · 5.1K citations

    31

    h-index

  2. Astronomy and Astrophysics

    17 publications · 1.1K citations

    16

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    16 publications · 1.1K citations

    13

    h-index

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

    PRD · 7 publications · 392 citations

    7

    h-index

  5. Physical Review Letters

    PRL · 7 publications · 1.4K citations

    7

    h-index

1–5