Wavelength-dependent Extinction

Wavelength-Dependent Extinction is a phenomenon in astrophysics wherein the attenuation of electromagnetic radiation by interstellar dust varies as a function of wavelength, characterized by greater extinction at shorter (bluer) wavelengths compared to longer (redder) wavelengths.

78

Publications

10.5K

Citations

276

Authors

166

Institutions

Publications per year

2017–2026

13

Authors

276

  1. LB
    Lars Biemann

    Heinrich Heine University Düsseldorf, Germany

    2 publications · 30 citations

    2

    h-index

  2. MM
    M. M. Kasliwal

    California Institute of Technology, United States

    2 publications · 142 citations

    2

    h-index

  3. TH
    Thomas Häber

    Karlsruhe Institute of Technology, Germany

    2 publications · 30 citations

    2

    h-index

  4. EL
    E. L. Fitzpatrick

    Villanova University, United States

    2 publications · 3.4K citations

    2

    h-index

  5. KK
    Karl Kleinermanns

    Heinrich Heine University Düsseldorf, Germany

    2 publications · 30 citations

    2

    h-index

1–5 of 276

Venues

  1. The Astrophysical Journal

    ApJ · 12 publications · 1.5K citations

    12

    h-index

  2. Applied Optics

    6 publications · 139 citations

    6

    h-index

  3. 3

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 2 publications · 3.2K citations

    2

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 2 publications · 49 citations

    2

    h-index

1–5