We perform a blinded cosmology analysis with cosmic shear two-point correlation functions
measured from more than 25 million galaxies in the Hyper Suprime-Cam three-year shear …

We present 108 full-sky gravitational lensing simulation data sets generated by performing
multiple-lens plane ray-tracing through high-resolution cosmological N-body simulations …

We constrain the scaling relation between optical richness (λ) and halo mass (M) for a
sample of Sloan Digital Sky Survey (SDSS) red-sequence Matched-filter Probabilistic …

We provide a new fitting formula of the matter bispectrum in the nonlinear regime calibrated
by high-resolution cosmological N-body simulations of 41 cold dark matter (wCDM, w …

We present the integrated three-point shear correlation function i ζ±–a higher order statistic
of the cosmic shear field–which can be directly estimated in wide-area weak lensing surveys …

Next-generation cosmological surveys will observe large portions of the sky, with significant
overlap between them. Multi-wavelength observations will enable us to analyse the same …

The integrated shear 3-point correlation function ζ±is a higher-order statistic of the cosmic
shear field that describes the modulation of the 2-point correlation function ξ±by long …

We present the integrated 3-point correlation functions (3PCF) involving both the cosmic
shear and the galaxy density fields. These are a set of higher-order statistics that describe …

We study the connection of matter density and its tracers from the probability density function
(PDF) perspective. One aspect of this connection is the conditional expectation value〈 …

Weak gravitational lensing convergence peaks, the local maxima in weak lensing
convergence maps, have been shown to contain valuable cosmological information …