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 …

The co-evolution between supermassive black holes and their environment is most directly
traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere …

The polarized thermal emission from diffuse Galactic dust is the main foreground present in
measurements of the polarization of the cosmic microwave background (CMB) at …

We present a comprehensive analysis of strong-lensing, weak-lensing shear and
magnification data for a sample of 16 X-ray-regular and 4 high-magnification galaxy clusters …

Observations of galaxies and galaxy clusters in the local universe can account for only∼
10% of the total baryon content. Cosmological simulations predict that the “missing baryons” …

This is the second in a series of papers studying the astrophysics and cosmology of
massive, dynamically relaxed galaxy clusters. The data set employed here consists of …

We present a new determination of the concentration–mass (c–M) relation for galaxy
clusters based on our comprehensive lensing analysis of 19 X-ray selected galaxy clusters …

We present a review of the current state of the art of cosmological dark matter simulations,
with particular emphasis on the implications for dark matter detection efforts and studies of …

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 …

Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic
web. As galaxies are accreted they are affected by their local environment before they enter …