In addition to the intrinsic clustering of galaxies themselves, the spatial distribution of
galaxies observed in surveys is modulated by the presence of weak lensing due to matter in …

As a Stage IV space-based telescope, the China Space Station Telescope (CSST) can
perform photometric and spectroscopic surveys simultaneously to explore the Universe …

One of the open issues of the standard cosmological model is the value of the cosmic dipole
measured from the Cosmic Microwave Background (CMB), as well as from the number count …

This work considers which higher order modeling effects on the cosmic shear angular power
spectra must be taken into account for Euclid. We identified the relevant terms and quantified …

The standard approach to test for deviations from general relativity on cosmological scales is
to combine measurements of the growth rate of structure with gravitational lensing. In this …

The EG statistic is a discriminating probe of gravity developed to test the prediction of
general relativity (GR) for the relation between gravitational potential and clustering on the …

The magnification of galaxies in modern galaxy surveys induces additional correlations in
the cosmic shear, galaxy–galaxy lensing, and clustering observables used in modern …

Galaxy surveys provide one of the best ways to constrain the theory of gravity at
cosmological scales. They can be used to constrain the two gravitational potentials …

We investigated a cosmological model that allows a momentum transfer between dark
matter and dark energy. The interaction in the dark sector mainly affects the behaviour of …

We present the halo number counts and its two-point statistics, the observable angular
power spectrum, extracted for the first time from relativistic N-body simulations. The halo …