As the largest virialized structures in the universe, galaxy clusters continue to grow and
accrete matter from the cosmic web. Due to the low gas density in the outskirts of clusters …

Until recently, only about 10% of the total intracluster gas volume had been studied with high
accuracy, leaving a vast region essentially unexplored. This is now changing and a wide …

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 …

The distribution of baryons provides a significant way to understand the formation of galaxy
clusters by revealing the details of its internal structure and changes over time. In this paper …

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We carry out a comprehensive Bayesian correlation analysis between hot halos and direct
masses of supermassive black holes (SMBHs), by retrieving the X-ray plasma properties …

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 …

Feedback processes from baryons are expected to strongly affect weak-lensing observables
of current and future cosmological surveys. In this paper we present a new parametrisation …

We characterized the population of galaxy clusters detected with the Sunyaev–Zeldovich
(SZ) effect with Planck by measuring the cool-core state of the objects in a well-defined …

Traditionally, galaxy clusters have been expected to retain all the material accreted since
their formation epoch. For this reason, their matter content should be representative of the …