Interstellar Dust Attenuation

Interstellar Dust Attenuation is a radiative transfer phenomenon in which ultraviolet light from extragalactic sources is selectively absorbed and scattered by interstellar dust grains, thereby reducing observed flux and altering spectral energy distributions in a wavelength-dependent manner.

158

Publications

14.6K

Citations

860

Authors

357

Institutions

Publications per year

2017–2026

77

Authors

860

  1. MB
    M. Baes

    Ghent University, Belgium

    11 publications · 506 citations

    11

    h-index

  2. SC
    S. Charlot

    Institut d'Astrophysique de Paris, France

    10 publications · 2.4K citations

    10

    h-index

  3. VB
    V. Buat

    Centre National de la Recherche Scientifique, France

    9 publications · 557 citations

    9

    h-index

  4. ZJ
    Zhiyuan Ji

    University of Arizona, United States

    7 publications · 441 citations

    7

    h-index

  5. SL
    Steven L. Finkelstein

    The University of Texas at Austin, United States

    7 publications · 476 citations

    7

    h-index

1–5 of 860

Venues

  1. The Astrophysical Journal

    ApJ · 52 publications · 6.3K citations

    35

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    46 publications · 3.4K citations

    33

    h-index

  3. Astronomy and Astrophysics

    19 publications · 914 citations

    18

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 678 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 5 publications · 347 citations

    5

    h-index

1–5