Cluster Lensing

Cluster Lensing is a type of gravitational lensing in which the collective mass of a galaxy cluster acts as a gravitational lens, distorting and magnifying the light from background galaxies through strong and weak lensing effects, enabling the study of dark matter distribution and high-redshift galaxy populations.

1K

Publications

69.1K

Citations

2.6K

Authors

679

Institutions

Publications per year

2017–2026

233

Variants

Galaxy Cluster Lensing

Authors

2.6K

  1. JK
    Jean‐Paul Kneib

    Centre National de la Recherche Scientifique, France

    74 publications · 7.1K citations

    49

    h-index

  2. TB
    Tom Broadhurst

    University of the Basque Country, Spain

    54 publications · 6.1K citations

    43

    h-index

  3. AZ
    Adi Zitrin

    Ben-Gurion University of the Negev, Israel

    68 publications · 6.7K citations

    42

    h-index

  4. MM
    M. Meneghetti

    Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy

    63 publications · 5.8K citations

    41

    h-index

  5. DC
    Dan Coe

    Space Telescope Science Institute, United States

    52 publications · 5.7K citations

    39

    h-index

1–5 of 2.6K

Venues

  1. The Astrophysical Journal

    ApJ · 342 publications · 29.6K citations

    93

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    274 publications · 15.8K citations

    69

    h-index

  3. Astronomy and Astrophysics

    122 publications · 6.8K citations

    50

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 30 publications · 1.6K citations

    22

    h-index

  5. The Astrophysical Journal Letters

    22 publications · 1.3K citations

    19

    h-index

1–5