Infrared Luminosity Functions

Infrared Luminosity Functions is a statistical construct in extragalactic infrared astronomy that describes the number density of galaxies per unit comoving volume per unit infrared luminosity interval, distinguishing it from related luminosity-based distributions by specifically quantifying the galaxy population's infrared-emitting properties as a function of luminosity.

534

Publications

49.2K

Citations

1.9K

Authors

529

Institutions

Publications per year

2017–2026

83

Variants

Infrared Luminosity Function

Authors

1.9K

  1. EL
    E. Le Floc’h

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    16 publications · 3.1K citations

    16

    h-index

  2. VB
    V. Buat

    Centre National de la Recherche Scientifique, France

    16 publications · 1.3K citations

    15

    h-index

  3. CG
    C. Gruppioni

    University of Bologna, Italy

    14 publications · 926 citations

    13

    h-index

  4. FP
    F. Pozzi

    University of Bologna, Italy

    14 publications · 1.2K citations

    13

    h-index

  5. TT
    Tsutomu T. Takeuchi

    Nagoya University, Japan

    14 publications · 693 citations

    13

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 214 publications · 21.6K citations

    76

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    112 publications · 9.1K citations

    49

    h-index

  3. Astronomy and Astrophysics

    59 publications · 4.5K citations

    36

    h-index

  4. The Astronomical Journal

    AJ · 43 publications · 4.5K citations

    30

    h-index

  5. The Astrophysical Journal Supplement Series

    11 publications · 4.3K citations

    11

    h-index

1–5