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

Publications

1.7K

Citations

369

Authors

130

Institutions

Publications per year

2017–2026

5

Authors

369

  1. OR
    O. Reimer

    Centre National de la Recherche Scientifique, France

    3 publications · 549 citations

    3

    h-index

  2. PF
    P. Fortin

    University of California, Santa Cruz, United States

    2 publications · 539 citations

    2

    h-index

  3. AR
    A. Reimer

    Centre National de la Recherche Scientifique, France

    2 publications · 539 citations

    2

    h-index

  4. RD
    R. Dubois

    Stanford University, United States

    2 publications · 539 citations

    2

    h-index

  5. JE
    J. E. Grove

    United States Naval Research Laboratory, United States

    2 publications · 539 citations

    2

    h-index

1–5 of 369

Venues

  1. Physical review. D/Physical review. D.

    PRD · 3 publications · 153 citations

    3

    h-index

  2. Nature

    3 publications · 63 citations

    3

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 3 publications · 212 citations

    3

    h-index

  4. 2

    h-index

  5. Astrophysics and Space Science

    2 publications · 33 citations

    2

    h-index

1–5