Redshift Measurement

Redshift Measurement is a quantitative astronomical technique that determines the dimensionless redshift parameter of celestial objects by analyzing the relative displacement of spectral features toward longer wavelengths, distinguishing it from other observational methods through its reliance on Doppler and cosmological principles to infer radial velocity and distance in extragalactic surveys.

2K

Publications

192.8K

Citations

9.3K

Authors

1.3K

Institutions

Publications per year

2017–2026

522

Authors

9.3K

  1. WJ
    Will J. Percival

    University of Portsmouth, United Kingdom

    61 publications · 10.2K citations

    42

    h-index

  2. AJ
    Ashley J. Ross

    University of Portsmouth, United Kingdom

    46 publications · 7.6K citations

    38

    h-index

  3. DJ
    David J. Schlegel

    Lawrence Berkeley National Laboratory, United States

    35 publications · 7.8K citations

    31

    h-index

  4. DJ
    Daniel J. Eisenstein

    Center for Astrophysics Harvard & Smithsonian, United States

    34 publications · 8.2K citations

    31

    h-index

  5. EG
    E. Gaztañaga

    Institute of Space Sciences, Spain

    40 publications · 3.5K citations

    30

    h-index

1–5 of 9.3K

Venues

  1. The Astrophysical Journal

    ApJ · 461 publications · 56.6K citations

    104

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    475 publications · 41.3K citations

    95

    h-index

  3. Astronomy and Astrophysics

    210 publications · 21.6K citations

    66

    h-index

  4. The Astronomical Journal

    AJ · 126 publications · 14.6K citations

    52

    h-index

  5. The Astrophysical Journal Supplement Series

    82 publications · 12.1K citations

    46

    h-index

1–5