This review presents a comprehensive overview of galaxy bias, that is, the statistical relation
between the distribution of galaxies and matter. We focus on large scales where cosmic …

Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound
overdensities in the initial density field and is accompanied by the most energetic …

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy
experiment that will study baryon acoustic oscillations (BAO) and the growth of structure …

We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

Studies of galaxy clusters have proved crucial in helping to establish the standard model of
cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis …

The scale-dependent bias effect on the galaxy power spectrum is a very promising probe of
the local primordial non-Gaussianity (PNG) parameter f NL, but the amplitude of the effect is …

The use of summary statistics beyond the two-point correlation function to analyse the non-
Gaussian clustering on small scales, and thereby, increasing the sensitivity to the underlying …

The simplest theory describing large-scale redshift-space distortions (RSD), based on linear
theory and distant galaxies, depends on the growth of cosmological structure, suggesting …

We investigate how much can be learnt about four types of primordial non-Gaussianity
(PNG) from small-scale measurements of the halo field. Using the quijote-png simulations …

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