Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

Abstract

We present a global measurement of the integrated Sachs-Wolfe (ISW) effect obtained by cross-correlating all relevant large scale galaxy data sets with the cosmic microwave background radiation map provided by the Wilkinson Microwave Anisotropy Probe. With these measurements, the overall ISW signal is detected at the ~ 4.5 sigma level. We also examine the cosmological implications of these measurements, particularly the dark energy equation of state w, its sound speed, and the overall curvature of the Universe. The flat LCDM model is a good fit to the data and, assuming this model, we find that the ISW data constrain Omega_m = 0.20 +0.19 -0.11 at the 95% confidence level. When we combine our ISW results with the latest baryon oscillation and supernovae measurements, we find that the result is still consistent with a flat LCDM model with w = -1 out to redshifts z > 1.

arXiv comment24 pages, 15 figures. Version accepted by PRD. Improved quasar data, revised parameter constraints

References in corpus (49)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• The Sloan Digital Sky Survey: Technical Summary
• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• The Sixth Data Release of the Sloan Digital Sky Survey
• 2MASS Extended Source Catalog: Overview and Algorithms
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
• Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• The Fifth Data Release of the Sloan Digital Sky Survey
• A correlation of the cosmic microwave sky with large scale structure
• Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
• Looking for $\Lambda$ with the Rees-Sciama Effect
• The shape of the SDSS DR5 galaxy power spectrum
• Detection of the ISW and SZ effects from the CMB-Galaxy correlation
• Cross-Correlation of the Cosmic Microwave Background with the 2MASS Galaxy Survey: Signatures of Dark Energy, Hot Gas, and Point Sources
• Efficient Photometric Selection of Quasars from the Sloan Digital Sky Survey: 100,000 z<3 Quasars from Data Release One
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources
• Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy
• First Measurement of the Clustering Evolution of Photometrically-Classified Quasars
• A high redshift detection of the integrated Sachs-Wolfe effect
• An alternative to the cosmological 'concordance model'
• Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
• Cross-correlation of WMAP 3rd year and the SDSS DR4 galaxy survey: new evidence for Dark Energy
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• The Physical Origin of Scale Dependent Bias in Cosmological Simulations
• Integrated Sachs-Wolfe effect in Cross-Correlation: The Observer's Manual
• Correlating the CMB with Luminous Red Galaxies : The Integrated Sachs-Wolfe Effect
• Measuring Dark Energy Clustering with CMB-Galaxy Correlations
• MegaZ-LRG: A photometric redshift catalogue of one million SDSS Luminous Red Galaxies
• Detection of the ISW effect and corresponding dark energy constraints
• Detection of the ISW effect and corresponding dark energy constraints made with directional spherical wavelets
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• Tracking Dark Energy with the ISW effect: short and long-term predictions
• Cross-correlating the Sloan Digital Sky Survey with the Microwave Sky
• Correlations Between the Cosmic X-ray and Microwave Backgrounds: Constraints on a Cosmological Constant
• Cross-Correlation of the Cosmic Microwave Background with Radio Sources: Constraints on an Accelerating Universe
• New light on Dark Cosmos
• The Large-Scale Structure of the X-ray Background and its Cosmological Implications
• Large-scale galaxy correlations as a test for dark energy
• New Constraint on Open Cold-Dark-Matter Models
• Chaplygin gas in light of recent Integrated Sachs--Wolfe effect data
• The large-scale bias of the hard X-ray background
• An indirect limit on the amplitude of primordial Gravitational Wave Background from CMB-Galaxy Cross Correlation

Cited by in corpus (222)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Modified Gravity and Cosmology
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Observational Probes of Cosmic Acceleration
• Cosmology and Fundamental Physics with the Euclid Satellite
• Challenges for $\Lambda$CDM: An update
• Cosmology and fundamental physics with the Euclid satellite
• Brane-World Gravity
• Dark Energy
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Testing General Relativity in Cosmology
• Approaches to Understanding Cosmic Acceleration
• Evidence for the accelerated expansion of the Universe from weak lensing tomography with COSMOS
• The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
• Breaking a Dark Degeneracy with Gravitational Waves
• Efficient Photometric Selection of Quasars from the Sloan Digital Sky Survey: II. ~1,000,000 Quasars from Data Release Six
• Radio and Millimeter Continuum Surveys and their Astrophysical Implications
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• The Carnegie Supernova Project: Second Photometry Data Release of Low-Redshift Type Ia Supernovae
• Searching for modified growth patterns with tomographic surveys
• Think Outside the Color Box: Probabilistic Target Selection and the SDSS-XDQSO Quasar Targeting Catalog
• Primordial non-gaussianity, statistics of collapsed objects, and the Integrated Sachs-Wolfe effect
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Constraining primordial non-Gaussianity with future galaxy surveys
• Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
• The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae
• Selecting Quasars by their Intrinsic Variability
• Probing modifications of General Relativity using current cosmological observations
• Constraints on f(R) gravity from probing the large-scale structure
• Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
• Ultra large-scale cosmology in next-generation experiments with single tracers
• Photometric redshifts and quasar probabilities from a single, data-driven generative model
• First-year Sloan Digital Sky Survey-II (SDSS-II) supernova results: consistency and constraints with other intermediate-redshift datasets
• Light propagation in statistically homogeneous and isotropic dust universes
• Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
• CMB lensing tomography with the DES Science Verification galaxies
• Past and present cosmic structure in the SDSS DR7 main sample
• Measuring the Speed of Dark: Detecting Dark Energy Perturbations
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Constraint on Coupled Dark Energy Models from Observations
• Cosmological Tests of General Relativity with Future Tomographic Surveys
• The significance of the integrated Sachs-Wolfe effect revisited
• Gravitational redshift and other redshift-space distortions of the imaginary part of the power spectrum
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• A Possible Cold Imprint of Voids on the Microwave Background Radiation
• The Color Variability of Quasars
• Investigating dark energy experiments with principal components
• Detecting the integrated Sachs-Wolfe effect with stacked voids
• Dissipation of dark matter
• Estimating the large-scale angular power spectrum in the presence of systematics: a case study of Sloan Digital Sky Survey quasars
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
• A model for the cosmological evolution of low frequency radio sources
• Observational Evidence of the Accelerated Expansion of the Universe
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• Shedding Light on the Galaxy Luminosity Function
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
• A WISE measurement of the ISW effect
• Tidal alignments as a contaminant of redshift space distortions
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Dark Energy in Practice
• Observational Evidence for Cosmological-Scale Extra Dimensions
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• A catalogue of photometric redshifts for the SDSS-DR9 galaxies
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogs
• The stacked ISW signal of rare superstructures in ΛCDM
• Measuring the Integrated Sachs-Wolfe Effect
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Quasar Probabilities and Redshifts from WISE mid-IR through GALEX UV Photometry
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• A Map of the Integrated Sachs-Wolfe Signal from Luminous Red Galaxies
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• Cosmological Measurements with Forthcoming Radio Continuum Surveys
• The High Redshift Integrated Sachs-Wolfe Effect
• Spherical collapse of dark energy with an arbitrary sound speed
• Observational Constraints on Kinetic Gravity Braiding from the Integrated Sachs-Wolfe Effect
• Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• A cross-correlation study of the Fermi-LAT $\gamma$-ray diffuse extragalactic signal
• Imprint of DES super-structures on the Cosmic Microwave Background
• Late universe dynamics with scale-independent linear couplings in the dark sector
• On structure formation from a small-scales-interacting dark sector
• Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
• Measurement of CIB power spectra over large sky areas from Planck HFI maps
• Machine Learning based photometric redshifts for the KiDS ESO DR2 galaxies
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Evidence against a supervoid causing the CMB Cold Spot
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• Integrated Sachs-Wolfe effect in massive bigravity
• Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys
• Revisiting the WMAP - NVSS angular cross correlation. A skeptic's view
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• What can CMB observations tell us about the neutrino distribution function?
• Detectability of a phantom-like braneworld model with the integrated Sachs-Wolfe effect
• Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
• Neutrino lumps and the Cosmic Microwave Background
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Residual Hubble-bubble effects on supernova cosmology
• ISW Imprint of Superstructures on Linear Scales
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Late time CMB anisotropies constrain mini-charged particles
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Mapping the Integrated Sachs-Wolfe Effect
• Phantom-like behaviour in a brane-world model with curvature effects
• The SDSS-III Baryonic Oscillation Spectroscopic Survey: Constraints on the Integrated Sachs Wolfe effect
• Towards accurate modelling of the ISW effect, the non-linear contribution
• Stacked CMB lensing and ISW signals around superstructures in the DESI Legacy Survey
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• The Parametrized Post-Newtonian-Vainshteinian Formalism
• Absence of significant cross-correlation between WMAP and SDSS
• Evolution in the bias of faint radio sources to z ~ 2.2
• The dark flow induced small scale kinetic Sunyaev Zel'dovich effect
• Stability of accelerating cosmology in two scalar-tensor theory: Little Rip versus de Sitter
• Statistical Classification Techniques for Photometric Supernova Typing
• Cosmological Density Fluctuations on 100Mpc Scales and their ISW Effect
• The integrated Sachs-Wolfe effect in cosmologies with coupled dark matter and dark energy
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Cold imprint of supervoids in the Cosmic Microwave Background re-considered with Planck and BOSS DR10
• The Integrated Sachs-Wolfe Signal from BOSS Super-Structures
• Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• Oscillating nonlinear large scale structure in growing neutrino quintessence
• Cross-correlation of WMAP7 and the WISE Full Data Release
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Large scale structure and ISW effect in decaying vacuum cosmology
• Could multiple voids explain the Cosmic Microwave Background Cold Spot anomaly?
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• A linear filter to reconstruct the ISW effect from CMB and LSS observations
• Growth of Matter Perturbations in the Bi-Galileons Field Model
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Measuring ISW with next-generation radio surveys
• Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey
• Integrated Cosmological Probes: Extended Analysis
• CMB-Galaxy correlation in Unified Dark Matter Scalar Field Cosmologies
• Lenses in the forest: cross-correlation of the Lyman-alpha flux with CMB lensing
• On Preferred Axes in WMAP Cosmic Microwave Background Data after Subtraction of the Integrated Sachs-Wolfe Effect
• Raytracing simulations of coupled dark energy models
• The Complementarity of Redshift-space Distortions and the Integrated Sachs-Wolfe Effect: A 3D Spherical Analysis
• The cross-correlation between 3d cosmic shear and the integrated Sachs-Wolfe effect
• Cosmological Probes of Structure Growth and Tests of Gravity
• Implications of bias evolution on measurements of the integrated Sachs-Wolfe effect: errors and biases in parameter estimation
• Testing model independent modified gravity with future large scale surveys
• Cross-correlation between the cosmic microwave and infrared backgrounds for integrated Sachs-Wolfe detection
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• Generalized Brans-Dicke theories in light of evolving dark energy
• Integrated Sachs-Wolfe map recovery from NVSS and WMAP 7yr data
• Parameter Estimation with BEAMS in the presence of biases and correlations
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• Peeling off the late Universe: Reconstructing the ISW map with galaxy surveys
• A gauge-invariant approach to interactions in the dark sector
• Integrated Sachs-Wolfe map reconstruction in the presence of systematic errors
• Mixed three-point correlation functions of the nonlinear integrated Sachs-Wolfe effect and their detectability
• A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data
• Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy
• ISW-LSS cross-correlation in coupled Dark Energy models with massive neutrinos
• Cosmology with the Square Kilometre Array by SKA-Japan
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Evolution of Spherical Overdensity in Thawing Dark energy Models
• Accelerated expansion of the universe and chasing photons from the CMB to study the late time integrated Sachs-Wolfe effect over different redshift ranges
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• The CMBR ISW and HI 21-cm Cross-correlation Angular Power Spectrum
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• Detecting the integrated Sachs-Wolfe effect with high-redshift 21-cm surveys
• Constraints on primordial non-Gaussianity from the cross-correlation of DESI Luminous Red Galaxies and $Planck$ CMB lensing
• Parameter estimation biases due to contributions from the Rees-Sciama effect to the integrated Sachs-Wolfe spectrum
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Cosmological constraints on dark energy
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• Rees--Sciama Effect and Impact of Foreground Structures on Galaxy Redshifts
• On the ISW-cluster cross-correlation in future surveys
• An improved estimator for non-Gaussianity in cosmic microwave background observations
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Improving CMB non-Gaussianity estimators using tracers of local structure
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Chaplygin gas in decelerating DGP gravity and the age of the oldest star
• Contributions to the nonlinear integrated Sachs-Wolfe effect: Birkinshaw-Gull effect and gravitational self-energy density
• Measurement of the baryonic acoustic oscillation scale in 21 cm intensity fluctuations during the reionisation era
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• Integrated Sachs-Wolfe tomography with orthogonal polynomials
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• Future Radio Continuum Cosmology Clustering Surveys
• Cross-correlating Planck with VST ATLAS LRGs: a new test for the ISW effect in the Southern Hemisphere
• Realizing the phantom-divide crossing with vector and scalar fields
• Measuring dark energy with the integrated Sachs-Wolfe effect
• Growing neutrino cosmology
• Detecting deviations from Gaussianity in high-redshift CMB lensing maps
• Theoretical Estimates of Integrated Sachs-Wolfe Effect Detection through EMU-ASKAP Survey with Confusion, Position Uncertainty, Shot Noise and SNR analysis
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
• Observations of General Relativity at strong and weak limits
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Cross bispectra and trispectra of the non-linear integrated Sachs-Wolfe effect and the tracer galaxy density field
• Uniformity of Cosmic Microwave Background as a Non-Inflationary Geometrical Effect
• Energy conditions and entropy density of the universe
• Inflationary epoch in the presence of holographic dark energy
• Impact of scale-dependent bias and nonlinear evolution on the ISW
• New Cosmological Model and Its Implications on Observational Data Interpretation
• Integrated Sachs-Wolfe maps from the Gower Street $w$CDM simulations
• Foreground Mitigation for CMB Lensing with the Global Minimum Variance Quadratic Estimator