Cluster Mass Estimation

Cluster Mass Estimation is a methodological framework in astrophysics that distinguishes itself by quantifying the total gravitational mass of galaxy clusters through observational proxies such as X-ray emission, Sunyaev-Zel'dovich effect, weak lensing, or velocity dispersion, thereby enabling cosmological inferences from large-scale structure.

1.3K

Publications

92.9K

Citations

4.2K

Authors

816

Institutions

Publications per year

2017–2026

275

Variants

Galaxy Cluster Mass Estimation

Authors

4.2K

  1. JM
    J. M. Diego

    Instituto de Física de Cantabria, Spain

    57 publications · 6.6K citations

    43

    h-index

  2. PB
    P. B. Lilje

    University of Oslo, Norway

    48 publications · 6.2K citations

    39

    h-index

  3. EM
    E. Martínez-González

    Instituto de Física de Cantabria, Spain

    48 publications · 6.1K citations

    39

    h-index

  4. SG
    S. Galeotta

    National Institute for Astrophysics, Italy

    46 publications · 6K citations

    38

    h-index

  5. ML
    M. López-Caniego

    Scuola Internazionale Superiore di Studi Avanzati, Italy

    46 publications · 6K citations

    38

    h-index

1–5 of 4.2K

Venues

  1. The Astrophysical Journal

    ApJ · 358 publications · 34K citations

    96

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    338 publications · 20.2K citations

    74

    h-index

  3. Astronomy and Astrophysics

    207 publications · 16.4K citations

    70

    h-index

  4. The Astronomical Journal

    AJ · 50 publications · 3.7K citations

    33

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 26 publications · 979 citations

    19

    h-index

1–5