Cluster Pressure Profiles

Cluster Pressure Profiles is a physical construct representing the radial distribution of intracluster medium pressure in galaxy clusters, derived from X-ray and Sunyaev-Zel'dovich observations, that distinguishes itself through its characterization of thermodynamic structure and its role in calibrating cosmological mass-observable relations.

208

Publications

16.6K

Citations

938

Authors

379

Institutions

Publications per year

2017–2026

69

Authors

938

  1. TM
    Tony Mroczkowski

    European Southern Observatory, Germany

    16 publications · 789 citations

    14

    h-index

  2. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    13 publications · 1.3K citations

    13

    h-index

  3. JS
    J. S. Sanders

    Max Planck Institute for Extraterrestrial Physics, Germany

    12 publications · 1.3K citations

    11

    h-index

  4. CL
    Craig L. Sarazin

    University of Virginia, United States

    11 publications · 843 citations

    11

    h-index

  5. MJ
    Mark J. Devlin

    University of Pennsylvania, United States

    10 publications · 438 citations

    10

    h-index

1–5 of 938

Venues

  1. Monthly Notices of the Royal Astronomical Society

    69 publications · 4.5K citations

    36

    h-index

  2. The Astrophysical Journal

    ApJ · 55 publications · 6.3K citations

    35

    h-index

  3. Astronomy and Astrophysics

    36 publications · 3K citations

    27

    h-index

  4. The Astrophysical Journal Letters

    10 publications · 278 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 8 publications · 258 citations

    8

    h-index

1–5