Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound
overdensities in the initial density field and is accompanied by the most energetic …

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 …

Aims. The eROSITA Final Equatorial-Depth Survey has been carried out during the
performance verification phase of the Spectrum-Roentgen-Gamma/eROSITA telescope and …

We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from
the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of …

We present cosmological parameter constraints based on the final nine-year Wilkinson
Microwave Anisotropy Probe (WMAP) data, in conjunction with a number of additional …

We detect a weak unidentified emission line at E=(3.55–3.57)±0.03 keV in a stacked XMM-
Newton spectrum of 73 galaxy clusters spanning a redshift range 0.01–0.35. When the full …

We present constraints on cosmological parameters using number counts as a function of
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …

The hypothesis that the late Universe is isotropic and homogeneous is adopted by most
cosmological studies, including studies of galaxy clusters. The cosmic expansion rate H 0 is …

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 the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …