Massive Galaxy Clusters

Massive Galaxy Clusters is a cosmological construct denoting the most gravitationally bound and massive assemblies of galaxies, dark matter, and hot intracluster gas, distinguished by their high X-ray luminosity, strong gravitational lensing effects, and role as probes of large-scale structure formation in the universe.

2.3K

Publications

176.4K

Citations

6K

Authors

1.1K

Institutions

Publications per year

2017–2026

652

Authors

6K

  1. HE
    H. Ebeling

    University of Hawaii System, United States

    59 publications · 8.6K citations

    48

    h-index

  2. JK
    Jean‐Paul Kneib

    Centre National de la Recherche Scientifique, France

    65 publications · 4.9K citations

    43

    h-index

  3. JJ
    J. J. Mohr

    Ludwig-Maximilians-Universität München, Germany

    52 publications · 5.8K citations

    35

    h-index

  4. AH
    Anthony H. Gonzalez

    University of Florida, United States

    47 publications · 3.9K citations

    34

    h-index

  5. JR
    Johan Richard

    Centre National de la Recherche Scientifique, France

    45 publications · 3.9K citations

    33

    h-index

1–5 of 6K

Venues

  1. The Astrophysical Journal

    ApJ · 644 publications · 56.1K citations

    126

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    701 publications · 54.5K citations

    116

    h-index

  3. Astronomy and Astrophysics

    275 publications · 16.2K citations

    69

    h-index

  4. The Astronomical Journal

    AJ · 69 publications · 6.2K citations

    41

    h-index

  5. The Astrophysical Journal Letters

    73 publications · 4.5K citations

    40

    h-index

1–5