Cluster Redshift Distribution

Cluster Redshift Distribution is a statistical construct in astrophysics that characterizes the frequency distribution of redshift values among galaxy clusters within a given survey or observational sample, serving to trace the large-scale structure and cosmic evolution of the universe.

519

Publications

32K

Citations

2.2K

Authors

544

Institutions

Publications per year

2017–2026

78

Authors

2.2K

  1. JJ
    J. J. Mohr

    Ludwig-Maximilians-Universität München, Germany

    17 publications · 1.8K citations

    17

    h-index

  2. DG
    D. Gruen

    Stanford University, United States

    16 publications · 1.1K citations

    15

    h-index

  3. TH
    T. H. Reiprich

    University of Bonn, Germany

    18 publications · 942 citations

    15

    h-index

  4. SG
    S. Grandis

    Ludwig-Maximilians-Universität München, Germany

    16 publications · 960 citations

    14

    h-index

  5. BM
    Bianca M. Poggianti

    Osservatorio Astronomico di Padova, Italy

    14 publications · 986 citations

    14

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 152 publications · 11.4K citations

    54

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    135 publications · 7.3K citations

    47

    h-index

  3. Astronomy and Astrophysics

    73 publications · 3.9K citations

    35

    h-index

  4. The Astronomical Journal

    AJ · 39 publications · 2.3K citations

    25

    h-index

  5. The Astrophysical Journal Supplement Series

    18 publications · 3K citations

    17

    h-index

1–5