[HTML][HTML] Large-scale galaxy bias
V Desjacques, D Jeong, F Schmidt - Physics reports, 2018 - Elsevier
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 …
between the distribution of galaxies and matter. We focus on large scales where cosmic …
Radio and millimeter continuum surveys and their astrophysical implications
G De Zotti, M Massardi, M Negrello, J Wall - The Astronomy and …, 2010 - Springer
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 …
from radio and millimeter sky surveys. Recent determinations of local luminosity functions …
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North
S Arnouts, S Cristiani, L Moscardini… - Monthly Notices of …, 1999 - academic.oup.com
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 …
correlation function and the photometric redshift distribution of galaxies brighter than I AB …
Cosmological analysis of three-dimensional BOSS galaxy clustering and Planck CMB lensing cross correlations via Lagrangian perturbation theory
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 …
clustering (RSD) and baryon acoustic oscillations (BAO) plus gravitational lensing (of the …
Galaxy evolution from halo occupation distribution modeling of DEEP2 and SDSS galaxy clustering
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 …
and SDSS (z~ 0) galaxies within the HOD framework. At both epochs, there is a tight …
Gravity and large-scale nonlocal bias
KC Chan, R Scoccimarro, RK Sheth - Physical Review D—Particles, Fields …, 2012 - APS
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 …
overdensities, bias, is most often assumed to be local at the time of observation in the large …
The large apex bolometer camera survey of the extended chandra deep field south
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 …
combining 310 hr of observing time with the Large Apex BOlometer Camera (LABOCA) on …
Stochastic nonlinear galaxy biasing
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 …
cosmological parameters, such as regression of light versus mass, the analysis of redshift …
Measuring the redshift evolution of clustering: the Hubble Deep Field South
S Arnouts, L Moscardini, E Vanzella… - Monthly Notices of …, 2002 - academic.oup.com
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 …
Hubble Deep Field South (HDF South). The HST optical data are combined with infrared …
The clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey
M White, AD Myers, NP Ross… - Monthly Notices of …, 2012 - academic.oup.com
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 …
using data from the Baryon Oscillation Spectroscopic Survey. We use a homogeneous …