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 measure weak lensing cosmic shear power spectra from the 3-year galaxy shear catalog
of the Hyper Suprime-Cam (HSC) Subaru Strategic Program imaging survey. The shear …

We present measurements of cosmic shear two-point correlation functions (TPCFs) from
Hyper Suprime-Cam Subaru Strategic Program (HSC) first-year data, and derive …

We present and characterize the catalog of galaxy shape measurements that will be used for
cosmological weak lensing measurements in the Wide layer of the first year of the Hyper …

We study weak gravitational lensing convergence maps produced from the MillenniumTNG
simulations by direct projection of the mass distribution on the past backwards lightcone of a …

We constrain the matter density Ωm and the amplitude of density fluctuations σ8 within the
ΛCDM cosmological model with shear peak statistics and angular convergence power …

Parameter estimation with non-Gaussian stochastic fields is a common challenge in
astrophysics and cosmology. In this paper, we advocate performing this task using the …

Weak lensing maps contain information beyond two-point statistics on small scales. Much
recent work has tried to extract this information through a range of different observables or …

Weak gravitational lensing is one of the most promising cosmological probes of the late
universe. Several large ongoing (DES, KiDS, HSC) and planned (LSST, Euclid, WFIRST) …

We present a proof-of-concept analysis of photometric redshifts with Bayesian priors on
physical properties of galaxies. This concept is particularly suited for upcoming/on-going …