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
Parents
208
M. Arnaud, G. W. Pratt, R. Piffaretti et al. · Astronomy and Astrophysics · 2010 · 958 citations · Full text
Natural Sciences, Astronomy, Physics +13
1–5 of 208
938
14
h-index
13
h-index
Max Planck Institute for Extraterrestrial Physics, Germany
12 publications · 1.3K citations
11
h-index
11
h-index
10
h-index
1–5 of 938
379
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
28 h-index
97 publications
13.4K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
27 h-index
50 publications
6.1K citations
Max Planck Institute for Astrophysics
Garching, Germany
21 h-index
44 publications
3.1K citations

Centre National de la Recherche Scientifique
Paris, France
20 h-index
238 publications
15.6K citations
University of Chicago
Chicago, United States
18 h-index
110 publications
9.3K citations
California Institute of Technology
Pasadena, United States
16 h-index
49 publications
3.5K citations
Max Planck Society
Munich, Germany
16 h-index
28 publications
3.9K citations
University of Pennsylvania
Philadelphia, United States
15 h-index
50 publications
2K citations
1–8 of 379
69 publications · 4.5K citations
36
h-index
ApJ · 55 publications · 6.3K citations
35
h-index
36 publications · 3K citations
27
h-index
10 publications · 278 citations
9
h-index
Repository · 8 publications · 258 citations
8
h-index
1–5