X-Ray Morphological Analysis of the Planck ESZ Clusters
L. Lovisari(Center for Astrophysics Harvard & Smithsonian), Ralph Kraft(Center for Astrophysics Harvard & Smithsonian), Scott W. Randall(Center for Astrophysics Harvard & Smithsonian), W. Forman(Center for Astrophysics Harvard & Smithsonian), Felipe Andrade-Santos(Center for Astrophysics Harvard & Smithsonian), S. Ettori(Osservatorio astronomico di Bologna), M. Arnaud(Centre National de la Recherche Scientifique), C. Jones(Smithsonian Astrophysical Observatory), G. W. Pratt(Centre National de la Recherche Scientifique), J. Démoclès(Centre National de la Recherche Scientifique)
Cited by 132
Related Papers
The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the<i>Y</i><sub>SZ</sub>–<i>M</i><sub>500</sub>relation
|Astronomy and Astrophysics|2010|956
Determination of confidence limits for experiments with low numbers of counts
|The Astrophysical Journal|1991|487
<i>Planck</i>intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
|Astronomy and Astrophysics|2015|415
Reflections of Active Galactic Nucleus Outbursts in the Gaseous Atmosphere of M87
|The Astrophysical Journal|2005|266
Evidence for heavy-seed origin of early supermassive black holes from a z ≈ 10 X-ray quasar
|Nature Astronomy|2023|247