Lyman Continuum Attenuation

Lyman Continuum Attenuation is a astrophysical phenomenon representing the reduction in intensity of far-ultraviolet photons below 912 Å due to absorption by neutral hydrogen and interstellar dust along the line of sight.

122

Publications

8.9K

Citations

472

Authors

219

Institutions

Publications per year

2017–2026

23

Authors

472

  1. DS
    D. Schaerer

    University of Geneva, Switzerland

    10 publications · 1.2K citations

    10

    h-index

  2. JC
    John Chisholm

    The University of Texas at Austin, United States

    6 publications · 540 citations

    6

    h-index

  3. AV
    Anne Verhamme

    Centre National de la Recherche Scientifique, France

    6 publications · 869 citations

    6

    h-index

  4. GW
    G. Worseck

    University of Potsdam, Germany

    5 publications · 808 citations

    5

    h-index

  5. HC
    Henry C. Ferguson

    Space Telescope Science Institute, United States

    5 publications · 613 citations

    5

    h-index

1–5 of 472

Venues

  1. The Astrophysical Journal

    ApJ · 39 publications · 4K citations

    29

    h-index

  2. 19

    h-index

  3. Astronomy and Astrophysics

    10 publications · 723 citations

    10

    h-index

  4. Nature

    5 publications · 404 citations

    5

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 4 publications · 86 citations

    4

    h-index

1–5