Diffuse Galactic Synchrotron Emission

Diffuse Galactic Synchrotron Emission is a type of pervasive, non-thermal radio emission originating from relativistic electrons spiraling in the Milky Way's magnetic field, distinguished by its smooth spatial distribution and spectral characteristics dominant at low frequencies.

89

Publications

5.1K

Citations

579

Authors

267

Institutions

Publications per year

2017–2026

23

Authors

579

  1. MH
    M. Haverkorn

    Radboud University Nijmegen, Netherlands

    8 publications · 391 citations

    8

    h-index

  2. CD
    C. Dickinson

    University of Manchester, United Kingdom

    7 publications · 768 citations

    7

    h-index

  3. GB
    G. Bernardi

    Rhodes University, South Africa

    7 publications · 391 citations

    7

    h-index

  4. JA
    J. Aumont

    Université Paris Cité, France

    6 publications · 476 citations

    6

    h-index

  5. ME
    Michael E. Jones

    University of Oxford, United Kingdom

    5 publications · 184 citations

    5

    h-index

1–5 of 579

Venues

  1. 16

    h-index

  2. Astronomy and Astrophysics

    16 publications · 1K citations

    15

    h-index

  3. The Astrophysical Journal

    ApJ · 16 publications · 1.7K citations

    14

    h-index

  4. Journal of Cosmology and Astroparticle Physics

    JCAP · 5 publications · 237 citations

    5

    h-index

  5. arXiv (Cornell University)

    Repository · 3 publications · 61 citations

    3

    h-index

1–5