Distance-redshift Relation

The Distance-Redshift Relation is a theoretical framework in cosmology that specifies the quantitative dependence of the proper distance to a celestial object on its cosmological redshift, uniquely encoding the expansion history of the universe through the integral of the inverse Hubble parameter over redshift.

700

Publications

54K

Citations

1.6K

Authors

623

Institutions

Publications per year

2017–2026

173

Authors

1.6K

  1. AS
    Allan Sandage

    Carnegie Observatories, United States

    19 publications · 2.4K citations

    18

    h-index

  2. TM
    T. M. Davis

    The University of Queensland, Australia

    12 publications · 2.1K citations

    12

    h-index

  3. BF
    Barry F. Madore

    Carnegie Observatories, United States

    8 publications · 1.8K citations

    8

    h-index

  4. KG
    Karl Glazebrook

    Swinburne University of Technology, Australia

    8 publications · 1.9K citations

    8

    h-index

  5. MW
    Martin White

    University of California, Berkeley, United States

    8 publications · 1.7K citations

    8

    h-index

1–5 of 1.6K

Venues

  1. The Astrophysical Journal

    ApJ · 136 publications · 11.4K citations

    60

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    101 publications · 12K citations

    41

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 70 publications · 3.4K citations

    36

    h-index

  4. 32

    h-index

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

    PRD · 31 publications · 1.4K citations

    24

    h-index

1–5