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 …

Weak gravitational lensing of background galaxies provides a direct probe of the projected
matter distribution in and around galaxy clusters. Here, we present a self-contained …

This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point
correlationfunctions of the cosmic microwave background (CMB) temperature and …

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 …

Masses of clusters of galaxies from weak gravitational lensing analyses of ever larger
samples are increasingly used as the reference to which baryonic scaling relations are …

We present a numerical study of dark matter halo concentrations in ΛCDM and self-similar
cosmologies. We show that the relation between concentration, c, and peak height, ν …

We present results from a comprehensive lensing analysis in Hubble Space Telescope
(HST) data of the complete Cluster Lensing And Supernova survey with Hubble cluster …

Large surveys of galaxy clusters with the Hubble Space Telescope (HST) and Spitzer,
including the Cluster Lensing And Supernova survey with Hubble and the Frontier Fields …

Gravitational lensing by clusters of galaxies offers a powerful probe of their structure and
mass distribution. Several research groups have developed techniques independently to …

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 …