Galaxy Redshift Distribution

Galaxy Redshift Distribution is a statistical construct in observational cosmology that characterizes the number density of galaxies as a function of their redshift, enabling the study of large-scale structure and cosmic evolution through the differentiation of galaxy populations across cosmological distances.

2.7K

Publications

238.9K

Citations

7.8K

Authors

1.2K

Institutions

Publications per year

2017–2026

496

Authors

7.8K

  1. WJ
    Will J. Percival

    University of Portsmouth, United Kingdom

    77 publications · 20.6K citations

    53

    h-index

  2. DJ
    Daniel J. Eisenstein

    Center for Astrophysics Harvard & Smithsonian, United States

    64 publications · 19.4K citations

    53

    h-index

  3. AJ
    Ashley J. Ross

    University of Portsmouth, United Kingdom

    64 publications · 16.2K citations

    50

    h-index

  4. DT
    D. Thomas

    University of Portsmouth, United Kingdom

    55 publications · 12.9K citations

    44

    h-index

  5. JP
    J. P. Huchra

    Center for Astrophysics Harvard & Smithsonian, United States

    56 publications · 6.8K citations

    42

    h-index

1–5 of 7.8K

Venues

  1. The Astrophysical Journal

    ApJ · 826 publications · 82K citations

    140

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    789 publications · 79.7K citations

    128

    h-index

  3. Astronomy and Astrophysics

    186 publications · 12K citations

    61

    h-index

  4. The Astronomical Journal

    AJ · 136 publications · 9.4K citations

    52

    h-index

  5. The Astrophysical Journal Supplement Series

    73 publications · 10.2K citations

    46

    h-index

1–5