Survey Geometry

Survey Geometry is a methodological construct in observational cosmology that specifies the three-dimensional spatial coverage and selection function of a redshift survey, distinguishing it by encoding the observable volume, angular and radial limits, and instrumental biases that govern the distribution of galaxies detectable within a given survey.

159

Publications

15.9K

Citations

849

Authors

356

Institutions

Publications per year

2017–2026

32

Authors

849

  1. IM
    I. Márquez

    Instituto de Astrofísica de Andalucía, Spain

    6 publications · 2.1K citations

    6

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    6 publications · 4.4K citations

    6

    h-index

  3. RM
    R. M. González Delgado

    Instituto de Astrofísica de Andalucía, Spain

    6 publications · 2.1K citations

    6

    h-index

  4. SF
    S. F. Sánchez

    Universidad Nacional Autónoma de México, Mexico

    6 publications · 2.1K citations

    6

    h-index

  5. DM
    D. Mast

    Instituto de Astrofísica de Andalucía, Spain

    6 publications · 2.1K citations

    6

    h-index

1–5 of 849

Venues

  1. Monthly Notices of the Royal Astronomical Society

    40 publications · 5.5K citations

    26

    h-index

  2. The Astrophysical Journal

    ApJ · 17 publications · 1.8K citations

    16

    h-index

  3. Astronomy and Astrophysics

    16 publications · 2.9K citations

    15

    h-index

  4. Journal of Cosmology and Astroparticle Physics

    JCAP · 11 publications · 448 citations

    11

    h-index

  5. 6

    h-index

1–5