The total mass of a galaxy cluster is one of its most fundamental properties. Together with
the redshift, the mass links observation and theory, allowing us to use the cluster population …

In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant
cosmological implications and have begun to serve as a powerful and independent probe of …

Context. The hot plasma in a galaxy cluster is expected to be heated to high temperatures
through shocks and adiabatic compression. The thermodynamical properties of the gas …

We describe the all-sky Planck catalogue of clusters and cluster candidates derived from
Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite …

We present the first results from romulusc, the highest resolution cosmological
hydrodynamic simulation of a galaxy cluster run to date. romulusc, a zoom-in simulation of a …

Aims. We present the reconstruction of hydrostatic mass profiles in 13 X-ray luminous galaxy
clusters that have been mapped in their X-ray and Sunyaev–Zeldovich (SZ) signals out to R …

Cosmological constraints from X-ray and microwave observations of galaxy clusters are
subjected to systematic uncertainties. Non-thermal pressure support due to internal gas …

The detailed velocity structure of the diffuse X-ray emitting intra-cluster medium (ICM)
remains one of the last missing key ingredients in understanding the microphysical …

We investigate the statistical properties and the origin of the scatter within the spatially
resolved surface brightness profiles of the CHEX–MATE sample, formed by 118 galaxy …

We report the scaling relations derived by fitting the X-ray parameters determined from
analyzing the XMM-Newton observations of 120 galaxy clusters in the Planck Early Sunyaev …