Extragalactic Radio Continuum

Extragalactic Radio Continuum is a non-thermal electromagnetic emission phenomenon in the radio frequency range originating from astrophysical sources outside the Milky Way Galaxy, distinguished by its diffuse synchrotron radiation mechanisms and absence of discrete spectral lines.

1.2K

Publications

67K

Citations

3.3K

Authors

751

Institutions

Publications per year

2017–2026

117

Authors

3.3K

  1. RB
    R. Beck

    Max Planck Institute for Radio Astronomy, Germany

    34 publications · 2K citations

    25

    h-index

  2. LF
    Luis F. Rodrı́guez

    Universidad Nacional Autónoma de México, Mexico

    24 publications · 2.5K citations

    19

    h-index

  3. MK
    M. Krause

    Max Planck Institute for Radio Astronomy, Germany

    21 publications · 1.3K citations

    19

    h-index

  4. GK
    G. K. Miley

    Leiden University, Netherlands

    19 publications · 1.9K citations

    18

    h-index

  5. RD
    R. D. Ekers

    Commonwealth Scientific and Industrial Research Organisation, Australia

    19 publications · 1.2K citations

    17

    h-index

1–5 of 3.3K

Venues

  1. The Astrophysical Journal

    ApJ · 383 publications · 19.8K citations

    73

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    189 publications · 9.4K citations

    56

    h-index

  3. Astronomy and Astrophysics

    131 publications · 7.2K citations

    47

    h-index

  4. The Astronomical Journal

    AJ · 120 publications · 5.4K citations

    41

    h-index

  5. Nature

    74 publications · 7.3K citations

    35

    h-index

1–5