Luminosity Function Evolution

Luminosity Function Evolution is a theoretical framework in galaxy evolution studies that characterizes the redshift-dependent changes in the number density of galaxies as a function of luminosity, distinguishing it from static luminosity functions by explicitly modeling how galaxy populations evolve across cosmic time.

1.4K

Publications

148.5K

Citations

3.4K

Authors

768

Institutions

Publications per year

2017–2026

212

Authors

3.4K

  1. GZ
    G. Zamorani

    University of Bologna, Italy

    35 publications · 4.2K citations

    32

    h-index

  2. HJ
    H. J. McCracken

    Institut d'Astrophysique de Paris, France

    24 publications · 3.7K citations

    23

    h-index

  3. OI
    O. Ilbert

    Centre National de la Recherche Scientifique, France

    20 publications · 2.9K citations

    20

    h-index

  4. LP
    L. Pozzetti

    University of Bologna, Italy

    19 publications · 2.9K citations

    19

    h-index

  5. AM
    Anton M. Koekemoer

    Space Telescope Science Institute, United States

    21 publications · 4.5K citations

    19

    h-index

1–5 of 3.4K

Venues

  1. The Astrophysical Journal

    ApJ · 509 publications · 60K citations

    116

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    404 publications · 44.5K citations

    105

    h-index

  3. Astronomy and Astrophysics

    108 publications · 10.1K citations

    55

    h-index

  4. The Astronomical Journal

    AJ · 67 publications · 8.6K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    27 publications · 2.4K citations

    22

    h-index

1–5