Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

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 …

We present cosmological parameter results from the final full-mission Planck measurements
of the cosmic microwave background (CMB) anisotropies, combining information from the …

We present cosmological parameter results from the final full-mission Planck measurements
of the CMB anisotropies. We find good consistency with the standard spatially-flat 6 …

The evolution of the large-scale distribution of matter is sensitive to a variety of fundamental
parameters that characterise the dark matter, dark energy, and other aspects of our …

Cold dark matter (CDM) constitutes most of the matter in the Universe. The interplay
between dark and luminous matter in dense cosmic environments, such as galaxy clusters …

We introduce the Cluster-EAGLE (c-eagle) simulation project, a set of cosmological
hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of …

We present a catalog of 182 galaxy clusters detected through the Sunyaev–Zel'dovich (SZ)
effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg 2 field. The clusters …

The plasma haloes filling massive galaxies, groups and clusters are shaped by active
galactic nucleus (AGN) heating and subsonic turbulence (σ v∼ 150 km s− 1), as probed by …

The fundamental properties of the postulated dark matter (DM) affect the internal structure of
gravitationally bound structures. In the cold dark matter paradigm, DM particles interact only …