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 …

We review the statistical properties of the main populations of radio sources, as emerging
from radio and millimeter sky surveys. Recent determinations of local luminosity functions …

The evolution of galaxy clustering from z= 0 to z≃ 4.5 is analysed using the angular
correlation function and the photometric redshift distribution of galaxies brighter than I AB …

We present a formalism for jointly fitting pre-and post-reconstruction redshift-space
clustering (RSD) and baryon acoustic oscillations (BAO) plus gravitational lensing (of the …

We model the luminosity-dependent projected two-point correlation function of DEEP2 (z~ 1)
and SDSS (z~ 0) galaxies within the HOD framework. At both epochs, there is a tight …

For Gaussian primordial fluctuations the relationship between galaxy and matter
overdensities, bias, is most often assumed to be local at the time of observation in the large …

We present a sensitive 870 μm survey of the Extended Chandra Deep Field South (ECDFS)
combining 310 hr of observing time with the Large Apex BOlometer Camera (LABOCA) on …

We propose a general formalism for galaxy biasing and apply it to methods for measuring
cosmological parameters, such as regression of light versus mass, the analysis of redshift …

We present an analysis of the evolution of galaxy clustering in the redshift interval in the
Hubble Deep Field South (HDF South). The HST optical data are combined with infrared …

We measure the quasar two-point correlation function over the redshift range 2.2< z< 2.8
using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous …