Cosmic shear is the distortion of images of distant galaxies due to weak gravitational lensing
by the large-scale structure in the Universe. Such images are coherently deformed by the …

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 …

We present cosmological results from a combined analysis of galaxy clustering and weak
gravitational lensing, using 1321 deg 2 of griz imaging data from the first year of the Dark …

We use 26× 10 6 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over
1321 deg 2 of the sky to produce the most significant measurement of cosmic shear in a …

We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters
selected from the Dark Energy Survey (DES) Year 1 dataset. Our analysis uses the same …

We present weak lensing shear catalogues from the fourth data release of the Kilo-Degree
Survey, KiDS-1000, spanning 1006 square degrees of deep and high-resolution imaging …

Metacalibration is a recently introduced method to accurately measure weak gravitational
lensing shear using only the available imaging data, without need for prior information about …

We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set,
covering 1500 deg2 with a median redshift of 0.59. The catalogues cover two main fields …

We constrain the mass–richness scaling relation of redMaPPer galaxy clusters identified in
the Dark Energy Survey Year 1 data using weak gravitational lensing. We split clusters into …

We present cosmological constraints from a joint cosmic shear analysis of the Kilo-Degree
Survey (KV450) and the Dark Energy Survey (DES-Y1), which were conducted using …