The Cluster HEritage project with XMM-Newton–Mass Assembly and Thermodynamics at
the Endpoint of structure formation (CHEX-MATE) is a three-mega-second Multi-Year …

Clusters of galaxies are useful tools to constrain cosmological parameters, only if their
masses can be correctly inferred from observations. In particular, X-ray and Sunyaev …

We present updated cosmological constraints from measurements of the gas mass fractions
(f gas) of massive, dynamically relaxed galaxy clusters. Our new data set has greater …

We use a set of about 300 simulated clusters from the three hundred Project to calculate
their hydrostatic masses and evaluate the associated bias by comparing them with the true …

We study the connection between morphology and dynamical state of the simulated galaxy
clusters in z∈[0, 1.031] from The Three Hundred project. We quantify cluster dynamical state …

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 …

Upcoming wide-field surveys are well suited to studying the growth of galaxy clusters by
tracing galaxy and gas accretion along cosmic filaments. We use hydrodynamic simulations …

Context. Galaxy clusters grow through the accretion of mass over cosmic time. Their
observed properties are then shaped by how baryons distribute and energy is diffused …

The relationship linking a galaxy cluster's total mass with the concentration of its mass profile
and its redshift is a fundamental prediction of the Cold Dark Matter (CDM) paradigm of …

We use the MACSIS hydrodynamical simulations to estimate the extent of gas clumping in
the intracluster medium of massive galaxy clusters and how it affects the hydrostatic mass …