The detection of the accelerated expansion of the Universe has been one of the major
breakthroughs in modern cosmology. Several cosmological probes (Cosmic Microwave …

We forecast constraints on primordial non-Gaussianity (PNG) and bias parameters from
measurements of galaxy power spectrum and bispectrum in future radio continuum and …

We comprehensively analyse the cosmology dependence of counts-in-cells statistics. We
focus on the shape of the one-point probability distribution function (PDF) of the matter …

We show that the anisotropies of the astrophysical stochastic gravitational wave background
in the mHz band have a strong dependence on the modelling of galactic and sub-galactic …

In the era of precision cosmology, establishing the correct magnitude of statistical errors in
cosmological parameters is of crucial importance. However, widely used approximations in …

Modified Gravity theories generally affect the Poisson equation and the gravitational slip in
an observable way, that can be parameterized by two generic functions (η and μ) of time and …

The angular power spectrum C ℓ (i, j) is a gauge-independent observable that is in principle
the natural tool for analysing galaxy number counts. In practice, the problem is that the …

Next-generation spectroscopic surveys such as the MegaMapper, MUltiplexed Survey
Telescope (MUST), MaunaKea Spectroscopic Explorer (MSE), and WideField Spectroscopic …

Future observations of the large-scale structure have the potential to investigate
cosmological models with a high degree of complexity, including the properties of gravity on …

We propose a methodology to measure the cosmological spatial curvature by employing the
deviation from statistical isotropy due to the Alcock-Paczy\'nski effect of large scale galaxy …