Survey Depth

Survey Depth is a metric in survey astronomy that quantifies the faintest apparent magnitude of celestial objects detectable by a given sky survey, distinguishing it from other survey characteristics by its focus on sensitivity limits rather than spatial coverage or resolution.

73

Publications

4.8K

Citations

728

Authors

316

Institutions

Publications per year

2017–2026

21

Variants

Limiting Magnitude

Authors

728

  1. RH
    Risa H. Wechsler

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    4 publications · 475 citations

    4

    h-index

  2. SD
    S. Desai

    University of Michigan, United States

    4 publications · 635 citations

    4

    h-index

  3. AE
    A. E. Evrard

    University of Michigan, United States

    4 publications · 401 citations

    4

    h-index

  4. RM
    R. Miquel

    Institute for High Energy Physics, Spain

    3 publications · 383 citations

    3

    h-index

  5. EB
    E. Bertin

    Institut d'Astrophysique de Paris, France

    3 publications · 625 citations

    3

    h-index

1–5 of 728

Venues

  1. The Astrophysical Journal

    ApJ · 14 publications · 1.1K citations

    13

    h-index

  2. 13

    h-index

  3. Astronomy and Astrophysics

    5 publications · 297 citations

    5

    h-index

  4. The Astrophysical Journal Supplement Series

    3 publications · 444 citations

    3

    h-index

  5. Publications of the Astronomical Society of Australia

    PASA · 2 publications · 259 citations

    2

    h-index

1–5