Galaxy shapes are not randomly oriented, rather they are statistically aligned in a way that
can depend on formation environment, history and galaxy type. Studying the alignment of …

Abstract The Baryon Oscillation Spectroscopic Survey (BOSS), part of the Sloan Digital Sky
Survey (SDSS) III project, has provided the largest survey of galaxy redshifts available to …

We evaluate the consistency between lensing and clustering based on measurements from
Baryon Oscillation Spectroscopic Survey combined with galaxy–galaxy lensing from Dark …

The first SRG/eROSITA All-Sky Survey (eRASS1) provides the largest intracluster medium-
selected galaxy cluster and group catalog covering the western Galactic hemisphere …

We present a study of the clustering and halo occupation distribution of Baryon Oscillation
Spectroscopic Survey (BOSS) CMASS galaxies in the redshift range 0.43< z< 0.7 drawn …

Strong gravitational lenses with measured time delays between the multiple images allow a
direct measurement of the time-delay distance to the lens, and thus a measure of …

The map** between the distributions of the observed galaxy stellar mass and the
underlying dark matter haloes provides the crucial link from theories of large-scale structure …

We analyze clustering measurements of BOSS galaxies using a simulation-based emulator
of two-point statistics. We focus on the monopole and quadrupole of the redshift-space …

Diffuse filaments connect galaxy clusters to form the cosmic web. Detecting these filaments
could yield information on the magnetic field strength, cosmic ray population, and …

We present the first weak-lensing mass calibration and X-ray scaling relations of galaxy
clusters and groups selected in the eROSITA Final Equatorial Depth Survey (eFEDS) …