Gamma-ray Sources

Gamma-Ray Sources is a class of astronomical objects or phenomena that emit electromagnetic radiation predominantly in the gamma-ray energy range, distinguished from other radiative sources by the extreme physical processes—such as cosmic ray interactions, relativistic particle acceleration, or nuclear transitions—that produce photons typically above 100 keV.

6.5K

Publications

407.7K

Citations

23.7K

Authors

2.5K

Institutions

Publications per year

2017–2026

1.2K

Authors

23.7K

  1. OR
    O. Reimer

    Centre National de la Recherche Scientifique, France

    217 publications · 35.4K citations

    96

    h-index

  2. DB
    D. Bastieri

    University of Padua, Italy

    176 publications · 31.9K citations

    93

    h-index

  3. DF
    D. F. Torres

    Institute of Space Sciences, Spain

    209 publications · 31.7K citations

    92

    h-index

  4. FL
    F. Longo

    University of Trieste, Italy

    223 publications · 32.2K citations

    92

    h-index

  5. AR
    A. Reimer

    Centre National de la Recherche Scientifique, France

    194 publications · 33.5K citations

    92

    h-index

1–5 of 23.7K

Venues

  1. The Astrophysical Journal

    ApJ · 1.6K publications · 123.5K citations

    159

    h-index

  2. Astronomy and Astrophysics

    472 publications · 28.5K citations

    85

    h-index

  3. Nature

    215 publications · 33.1K citations

    83

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    427 publications · 28K citations

    78

    h-index

  5. The Astrophysical Journal Letters

    187 publications · 12.7K citations

    64

    h-index

1–5