The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions

Abstract

Higher-order statistics are a useful and complementary tool for measuring the clustering of galaxies, containing information on the non-gaussian evolution and morphology of large-scale structure in the Universe. In this work we present measurements of the three-point correlation function (3PCF) for 187,000 galaxies in the WiggleZ spectroscopic galaxy survey. We explore the WiggleZ 3PCF scale and shape dependence at three different epochs z=0.35, 0.55 and 0.68, the highest redshifts where these measurements have been made to date. Using N-body simulations to predict the clustering of dark matter, we constrain the linear and non-linear bias parameters of WiggleZ galaxies with respect to dark matter, and marginalise over them to obtain constraints on sigma_8(z), the variance of perturbations on a scale of 8 Mpc/h and its evolution with redshift. These measurements of sigma_8(z), which have 10-20% accuracies, are consistent with the predictions of the LCDM concordance cosmology and test this model in a new way.

MNRAS Accepted, 16 pages, 18 figures

References in corpus (59)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Populating a cluster of galaxies - I. Results at z=0
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Halo Models of Large Scale Structure
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Using the Evolution of Clusters to Constrain Omega
• The Fourth Data Release of the Sloan Digital Sky Survey
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• The Luminosity and Color Dependence of the Galaxy Correlation Function
• Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
• A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• The WiggleZ Dark Energy Survey: Survey Design and First Data Release
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• Cosmological Constraints from the SDSS maxBCG Cluster Catalog
• Biasing and Hierarchical Statistics in Large-scale Structure
• The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
• Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime
• Parameterized Beyond-Einstein Growth
• CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing
• The Bispectrum as a Signature of Gravitational Instability in Redshift-Space
• The shape of the SDSS DR5 galaxy power spectrum
• The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z=0.6
• The Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG Sample
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
• The Red-sequence Cluster Survey-2 (RCS-2): survey details and photometric catalog construction
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS
• The Effect of Large-Scale Structure on the SDSS Galaxy Three-Point Correlation Function
• The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
• The 3-point function in large scale structure: redshift distortions and galaxy bias
• Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
• An analytic model for the bispectrum of galaxies in redshift space
• The Three-point Correlation Function of Galaxies Determined from the 2dF Galaxy Redshift Survey
• Three-point Correlation Functions of SDSS Galaxies in Redshift Space: Morphology, Color, and Luminosity Dependence
• The Three-point Function as a Probe of Models for Large-scale Structure
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• The SDSS Coadd: Cosmic Shear Measurement
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function
• The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey
• Modeling the three-point correlation function
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• Measuring our universe from galaxy redshift surveys
• The 3-point function in the large scale structure: I. The weakly non-linear regime in N-body simulations
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Precision Measurements of Higher-Order Angular Galaxy Correlations Using 11 Million SDSS Galaxies
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• The WiggleZ Dark Energy Survey: Galaxy Evolution at 0.25 < z < 0.75 Using The Second Red-Sequence Cluster Survey (RCS-2)

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• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
• Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity
• Constraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies
• Assessment of the Information Content of the Power Spectrum and Bispectrum
• A deep learning approach to cosmological dark energy models
• Precision analysis of the redshift-space galaxy bispectrum
• A complete FFT-based decomposition formalism for the redshift-space bispectrum
• Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
• Dark Sky Simulations: Early Data Release
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Fast and accurate mock catalogue generation for low-mass galaxies
• Near optimal bispectrum estimators for large-scale structure
• Measuring the growth of matter fluctuations with third-order galaxy correlations
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• Voids in the SDSS DR9: observations, simulations, and the impact of the survey mask
• The BOSS-WiggleZ overlap region I: Baryon Acoustic Oscillations
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies
• Probing Dark Energy through Scale Dependence
• Galaxy filaments as pearl necklaces
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Mitigating contamination in LSS surveys: a comparison of methods
• Modelling The Redshift-Space Three-Point Correlation Function in SDSS-III
• Polarization of a stochastic gravitational wave background through diffusion by massive structures
• The dark matter of galaxy voids
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Position-dependent correlation function from the SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 10 CMASS Sample
• Information Content of Higher-Order Galaxy Correlation Functions
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• What Can We Learn by Combining the Skew Spectrum and the Power Spectrum?
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• The locations of halo formation and the peaks formalism
• Non-local bias contribution to third-order galaxy correlations
• A new method to measure galaxy bias
• Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• The HI intensity mapping bispectrum including observational effects
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Toward Accurate Modeling of the Nonlinear Matter Bispectrum: Standard Perturbation Theory and Transients from Initial Conditions
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Efficient parallel algorithm for estimating higher-order polyspectra
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: higher-order correlations revealed by germ-grain Minkowski Functionals
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• The Integrated Bispectrum in Modified Gravity Theories
• Measurement of the Cross-Correlation Angular Power Spectrum Between the Stochastic Gravitational Wave Background and Galaxy Over-Density
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
• Consistency Relations in Effective Field Theory
• Higher multipoles of the galaxy bispectrum in redshift space
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• Antisymmetric galaxy cross-correlations as a cosmological probe
• RCSLenS: A new estimator for large-scale galaxy-matter correlations
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• On the Fast Random Sampling and Other Properties of the Three Point Correlation Function in Galaxy Surveys
• Cosmological surveys with multi-object spectrographs
• Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
• Non-Gaussianity in DHOST inflation
• Measuring anisotropies in the PTA band with cross-correlations
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• Probing cosmology via the clustering of critical points
• Bayesian deep learning for dark energy
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• Cross correlations of the CMB Doppler mode and the 21 cm brightness temperature in the presence of a primordial magnetic field
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• Obtaining non-linear galaxy bias constraints from galaxy-lensing phase differences
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space