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

The precise estimation of the mass of galaxy clusters is a major issue for cosmology. Large
galaxy cluster surveys rely on scaling laws that relate cluster observables to their masses …

We present panco2, an open-source Python library designed to extract galaxy cluster
pressure profiles from maps of the thermal Sunyaev-Zeldovich effect. The extraction is based …

An accurate reconstruction of galaxy cluster masses is key to use this population of objects
as a cosmological probe. In this work we present a study on the hydrostatic-to-lensing mass …

In this paper, we propose a self-consistent test for a Hubble constant estimate using galaxy
cluster and type Ia supernovae (SNe Ia) observations. The approach consists, in a first step …

Having a detailed knowledge of the intracluster medium (ICM) to infer the exact cluster
physics such as the cluster dynamical state is crucial for cluster-based cosmological studies …

The determination of the mass of galaxy clusters from observations is subject to systematic
uncertainties. Beyond the errors due to instrumental and observational systematic effects, in …

Recently, Odrzywolek and Rafelski (arxiv: 1612.03556) have found three distinct categories
of exoplanets, when they are classified based on density. We first carry out a similar …

Synthetic datasets generated from large-volume gravity-only simulations are an important
tool in the calibration of cosmological analyses. Their creation often requires accurate …

The abundance of galaxy clusters with mass and redshift is a wellknown cosmological
probe. The cluster mass is a key parameter for studies that aim to constrain cosmological …