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 …

Measurements of the clustering of galaxies in Fourier space, and at low wavenumbers, offer
a window into the early Universe via the possible presence of scale dependent bias …

We determine the number counts to second order in cosmological perturbation theory in the
Poisson gauge and allowing for anisotropic stress. The calculation is performed using an …

The large scale limit of the galaxy power spectrum provides a unique window into the early
Universe through a possible detection of scale dependent bias produced by primordial non …

The statistics of primordial curvature fluctuations are our window into the period of inflation,
where these fluctuations were generated. To date, the cosmic microwave background has …

Galaxy power spectrum and bispectrum signals are distorted by peculiar velocities and other
relativistic effects arising from a perturbed spacetime background. In addition, study of …

We study the power spectrum dipole of an N-body simulation which includes relativistic
effects through ray-tracing and covers the low redshift Universe up to z max= 0.465 …

Primordial non-Gaussianities (PNG) leave unique signatures in the bispectrum of the large-
scale structure. With upcoming galaxy surveys set to improve PNG constraints by at least …

We investigate how the lensing potential can be measured tomographically with future
galaxy surveys using their number counts. Such a measurement is an independent test of …

We discuss the dominant terms of the relativistic galaxy number counts to second order in
cosmological perturbation theory on sub-Hubble scales and on intermediate to large …