Galaxy Bias

Galaxy Bias is a theoretical construct in cosmology that quantifies the difference between the spatial distribution of galaxies and the underlying dark matter density field, serving as a proportionality factor that relates fluctuations in galaxy number counts to matter overdensities on large scales.

770

Publications

60.4K

Citations

2.2K

Authors

576

Institutions

Publications per year

2017–2026

225

Authors

2.2K

  1. EG
    E. Gaztañaga

    Institute of Space Sciences, Spain

    34 publications · 1.9K citations

    24

    h-index

  2. WJ
    Will J. Percival

    University of Portsmouth, United Kingdom

    31 publications · 3.2K citations

    24

    h-index

  3. MC
    M. Crocce

    Institute of Space Sciences, Spain

    28 publications · 2.5K citations

    22

    h-index

  4. AJ
    Ashley J. Ross

    University of Portsmouth, United Kingdom

    25 publications · 1.8K citations

    20

    h-index

  5. OL
    O. Lahav

    University College London, United Kingdom

    21 publications · 1.5K citations

    19

    h-index

1–5 of 2.2K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    262 publications · 18.5K citations

    74

    h-index

  2. The Astrophysical Journal

    ApJ · 159 publications · 17K citations

    66

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 82 publications · 5K citations

    38

    h-index

  4. 33

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 29 publications · 1.8K citations

    24

    h-index

1–5