Galaxy Color Evolution

Galaxy Color Evolution is a theoretical construct in astrophysics that characterizes the systematic change in the integrated optical and near-infrared spectral energy distributions of galaxies over cosmic time, primarily driven by variations in stellar populations, star formation histories, and dust attenuation.

1K

Publications

89.5K

Citations

2.8K

Authors

700

Institutions

Publications per year

2017–2026

127

Authors

2.8K

  1. MF
    Marijn Franx

    Leiden University, Netherlands

    22 publications · 2.8K citations

    22

    h-index

  2. GZ
    G. Zamorani

    University of Bologna, Italy

    24 publications · 1.5K citations

    21

    h-index

  3. HJ
    H. J. McCracken

    Institut d'Astrophysique de Paris, France

    21 publications · 1.5K citations

    20

    h-index

  4. MB
    M. Bolzonella

    University of Bologna, Italy

    21 publications · 1.1K citations

    19

    h-index

  5. AM
    Anton M. Koekemoer

    Space Telescope Science Institute, United States

    20 publications · 1.8K citations

    19

    h-index

1–5 of 2.8K

Venues

  1. The Astrophysical Journal

    ApJ · 348 publications · 39.8K citations

    103

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    243 publications · 17.4K citations

    71

    h-index

  3. The Astronomical Journal

    AJ · 93 publications · 11.5K citations

    45

    h-index

  4. Astronomy and Astrophysics

    84 publications · 4.5K citations

    41

    h-index

  5. The Astrophysical Journal Supplement Series

    24 publications · 3.1K citations

    22

    h-index

1–5