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 current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …

We present cluster counts and corresponding cosmological constraints from the Planck full
mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev …

We use the largest sample of z 6~ galaxies to date from the first four Hubble Frontier Fields
clusters to set constraints on the shape of the z 6~ luminosity functions (LFs) to fainter than M …

We perform numerical simulations of the merging galaxy cluster 1E 0657-56 (the Bullet
Cluster), including the effects of elastic dark matter scattering. In a similar manner to the …

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

CLASH: JOINT ANALYSIS OF STRONG-LENSING, WEAK-LENSING SHEAR, AND
MAGNIFICATION DATA FOR 20 GALAXY CLUSTERS - IOPscience Skip to content IOP …

We analyse strongly lensed images in eight galaxy clusters to measure their dark matter
density profiles in the radial region between 10 kpc and 150 kpc, and use this to constrain …

We introduce the the three hundred project, an endeavour to model 324 large galaxy
clusters with full-physics hydrodynamical re-simulations. Here we present the data set and …

Profiles of dark matter-dominated halos at the group and cluster scales play an important
role in modern cosmology. Using results from two very large cosmological N-body …