Galactic Dust Attenuation

Galactic Dust Attenuation is a physical process in astrophysics whereby interstellar dust grains within the Milky Way preferentially absorb and scatter shorter-wavelength electromagnetic radiation, thereby diminishing the observed flux and reddening the spectral energy distribution of background astronomical sources.

177

Publications

16.2K

Citations

893

Authors

342

Institutions

Publications per year

2017–2026

83

Authors

893

  1. VB
    V. Buat

    Centre National de la Recherche Scientifique, France

    10 publications · 821 citations

    10

    h-index

  2. BD
    Benjamin D. Johnson

    Center for Astrophysics Harvard & Smithsonian, United States

    9 publications · 1.2K citations

    9

    h-index

  3. ST
    Sandro Tacchella

    University of Cambridge, United Kingdom

    8 publications · 953 citations

    8

    h-index

  4. SP
    Simon P. Driver

    The University of Western Australia, Australia

    8 publications · 613 citations

    8

    h-index

  5. JI
    J. Iglésias-Páramo

    Instituto de Astrofísica de Andalucía, Spain

    7 publications · 565 citations

    7

    h-index

1–5 of 893

Venues

  1. The Astrophysical Journal

    ApJ · 56 publications · 6.8K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    59 publications · 4.2K citations

    38

    h-index

  3. Astronomy and Astrophysics

    14 publications · 906 citations

    13

    h-index

  4. The Astrophysical Journal Supplement Series

    6 publications · 1.9K citations

    6

    h-index

  5. The Astrophysical Journal Letters

    5 publications · 581 citations

    5

    h-index

1–5