Luminosity Function Of Galaxies

The "Luminosity Function of Galaxies" is a statistical model in astrophysics that describes the number density of galaxies per unit luminosity interval, distinguishing it from other galaxy distribution models by quantifying how galaxy populations vary with intrinsic brightness in a given volume of space.

2K

Publications

190.7K

Citations

4.2K

Authors

863

Institutions

Publications per year

2017–2026

264

Variants

Galaxy Luminosity FunctionGlf

Authors

4.2K

  1. CS
    Carlos S. Frenk

    Durham University, United Kingdom

    33 publications · 7.2K citations

    31

    h-index

  2. SP
    Simon P. Driver

    The University of Western Australia, Australia

    35 publications · 5.6K citations

    29

    h-index

  3. GZ
    G. Zamorani

    University of Bologna, Italy

    32 publications · 2.6K citations

    26

    h-index

  4. CM
    C. M. Baugh

    Durham University, United Kingdom

    29 publications · 6K citations

    25

    h-index

  5. RS
    Richard S. Ellis

    California Institute of Technology, United States

    24 publications · 5.8K citations

    24

    h-index

1–5 of 4.2K

Venues

  1. The Astrophysical Journal

    ApJ · 734 publications · 78K citations

    140

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    514 publications · 48.1K citations

    115

    h-index

  3. The Astronomical Journal

    AJ · 178 publications · 20.1K citations

    73

    h-index

  4. Astronomy and Astrophysics

    146 publications · 9.3K citations

    58

    h-index

  5. The Astrophysical Journal Supplement Series

    44 publications · 8.2K citations

    32

    h-index

1–5