Absorption Line Saturation

Absorption Line Saturation is an astrophysical phenomenon in spectroscopy where the equivalent width of an absorption line ceases to increase linearly with column density due to the line core reaching maximum opacity, thereby limiting the quantitative analysis of interstellar material.

121

Publications

5.8K

Citations

358

Authors

152

Institutions

Publications per year

2017–2026

9

Variants

Spectral Line Saturation

Authors

358

  1. FH
    Fred Hamann

    University of Florida, United States

    6 publications · 321 citations

    6

    h-index

  2. BD
    Blair D. Savage

    University of Wisconsin–Madison, United States

    5 publications · 866 citations

    5

    h-index

  3. TM
    Todd M. Tripp

    University of Massachusetts Amherst, United States

    4 publications · 235 citations

    4

    h-index

  4. PC
    Ph. Cahuzac

    Laboratoire Aimé Cotton, France

    3 publications · 65 citations

    3

    h-index

  5. LL
    Limin Lu

    California Institute of Technology, United States

    3 publications · 131 citations

    3

    h-index

1–5 of 358

Venues

  1. The Astrophysical Journal

    ApJ · 21 publications · 1.8K citations

    17

    h-index

  2. 9

    h-index

  3. Optics Communications

    7 publications · 205 citations

    7

    h-index

  4. Applied Physics Letters

    7 publications · 395 citations

    7

    h-index

  5. IEEE Journal of Quantum Electronics

    5 publications · 137 citations

    5

    h-index

1–5