We introduce the new TNG-Cluster project, an addition to the IllustrisTNG suite of
cosmological magnetohydrodynamical simulations of galaxy formation. Our objective is to …

A classification of the galaxy cluster's dynamical state is crucial when dealing with large
samples. The identification of the most relaxed and most disturbed objects is necessary for …

We present a catalog of 689 galaxy cluster candidates detected at significance $\xi> 4$ via
their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500 …

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 …

The intra-cluster medium is prone to turbulent motion that will contribute to the non-thermal
heating of the gas, complicating the use of galaxy clusters as cosmological probes. Indirect …

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 …

Matter distribution around clusters is highly anisotropic because clusters are the nodes of
the cosmic web. The shape of the clusters and the number of filaments to which they are …

Context. Turbulent processes at work in the intracluster medium perturb this environments,
impacting its properties, displacing gas, and creating local density fluctuations that can be …

ABSTRACT The relativistic Sunyaev-Zel'dovich (SZ) effect can be used to measure
intracluster gas temperatures independently of X-ray spectroscopy. Here, we use the large …

Matter distribution in the environment of galaxy clusters, from their cores to their connected
cosmic filaments, must in principle be related to the underlying cluster physics and its …