Diffuse Galactic Light

Diffuse Galactic Light is a component of diffuse sky radiation that originates from starlight scattered by interstellar dust grains distributed throughout the Milky Way, distinguished from other galactic emissions by its extended, non-localized spatial profile and wavelength-dependent polarization characteristics.

101

Publications

8.1K

Citations

325

Authors

192

Institutions

Publications per year

2017–2026

19

Authors

325

  1. KT
    Kohji Tsumura

    Japan Aerospace Exploration Agency, Japan

    6 publications · 264 citations

    6

    h-index

  2. SM
    Shuji Matsuura

    Institute of Space and Astronautical Science, Japan

    6 publications · 243 citations

    6

    h-index

  3. TM
    Toshio Matsumoto

    Institute of Space and Astronautical Science, Japan

    5 publications · 230 citations

    5

    h-index

  4. MA
    M. Arnaboldi

    Astronomical Observatory of Capodimonte, Italy

    4 publications · 129 citations

    4

    h-index

  5. AN
    Adolf N. Witt

    University of Toledo, United States

    4 publications · 309 citations

    4

    h-index

1–5 of 325

Venues

  1. The Astrophysical Journal

    ApJ · 40 publications · 5.2K citations

    29

    h-index

  2. 13

    h-index

  3. Astronomy and Astrophysics

    9 publications · 568 citations

    9

    h-index

  4. The Astronomical Journal

    AJ · 6 publications · 300 citations

    6

    h-index

  5. arXiv (Cornell University)

    Repository · 3 publications · 68 citations

    3

    h-index

1–5