Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization

Abstract

The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the full sky in Stokes I, Q, and U parameters at frequencies 23, 33, 41, 61, and 94 GHz. We detect correlations between the temperature and polarization maps significant at more than 10 standard deviations. The correlations are present in all WMAP frequency bands with similar amplitude from 23 to 94 GHz, and are consistent with a superposition of a CMB signal with a weak foreground. The fitted CMB component is robust against different data combinations and fitting techniques. On small angular scales theta < 5 deg, the WMAP data show the temperature-polarization correlation expected from adiabatic perturbations in the temperature power spectrum. The data for l > 20 agree well with the signal predicted solely from the temperature power spectra, with no additional free parameters. We detect excess power on large angular scales (theta > 10 deg) compared to predictions based on the temperature power spectra alone. The excess power is well described by reionization at redshift 11 < z_r < 30 at 95% confidence, depending on the ionization history. A model-independent fit to reionization optical depth yields results consistent with the best-fit LambdaCDM model, with best fit value tau = 0.17 +- 0.04 at 68% confidence, including systematic and foreground uncertainties. This value is larger than expected given the detection of a Gunn-Peterson trough in the absorption spectra of distant quasars, and implies that the universe has a complex ionization history: WMAP has detected the signal from an early epoch of reionization.

Replaced with version accepted by ApJ; Fig. 9 caption fixed. One of 13 companion papers on first-year WMAP results; 33 pages, 9 figures; version with higher quality figures is at http://lambda.gsfc.nasa.gov/

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• Compact radio cores: from the first black holes to the last
• 21 cm Tomography of the High-Redshift Universe with the Square Kilometer Array
• The Ionizing Efficiency of the First Stars
• AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
• Redshift space 21 cm power spectra from reionization
• Population III Star Formation in a Lambda WDM Universe
• Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
• Top-Down Fragmentation of a Warm Dark Matter Filament
• The Space Density of Redshift 5.7 Ly-Alpha Emitters
• Revisiting the Constraint on the Helium Abundance from CMB
• The Yuan-Tseh Lee Array for Microwave Background Anisotropy
• Free-Free Emission at Low Radio Frequencies
• Can Planck-scale physics be seen in the cosmic microwave background ?
• An upper limit to polarized submillimetre emission in Arp 220
• Extracting cosmic microwave background polarisation from satellite astrophysical maps
• Probing the Universe on Gigaparsec Scales with Remote Cosmic Microwave Background Quadrupole Measurements
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• CMB constraints on the fine structure constant
• Clarifying Inflation Models: Slow-roll as an expansion in 1/N_{efolds}
• Precision Cosmology
• Coupling Quintessence to Inflation in Supergravity
• Hubble Advanced Camera for Surveys Observations of the z=6.42 Quasar SDSS 1148+5251: A Leak in the Gunn-Peterson Trough
• The Redshift Distribution of Distant Supernovae and its Use in Probing Reionization
• Deconvolution Map-Making for Cosmic Microwave Background Observations
• Diffuse Cosmic Neutrino Background from Population III Stars
• On spatial distributions of old globular clusters in clusters of galaxies
• Inference for eigenvalues and eigenvectors of Gaussian symmetric matrices
• Adaptive Mesh Refinement Simulations of the Ionization Structure and Kinematics of Damped Ly$\alpha$ Systems with Self-consistent Radiative Transfer
• Partially ionizing the universe by decaying particles
• Dark Matter and Dark Energy from a single scalar field and CMB data
• Forming supermassive black holes by accreting dark and baryon matter
• Direct Wavelet Expansion of the Primordial Power Spectrum
• Reconstructing the Primordial Spectrum with CMB Temperature and Polarization
• On the road to discovery of relic gravitational waves: The TE and BB Correlations in the cosmic microwave background radiation
• Did Massive Primordial Stars Preenrich the Lyman Alpha Forest?
• Patchy He II reionization and the physical state of the IGM
• Measuring Statistical Isotropy of CMB Anisotropy
• Formation of intracluster globular clusters
• Cosmological perturbations and noncommutative tachyon inflation
• Cosmic backgrounds due to the formation of the first generation of supermassive black holes
• A search for low surface brightness dwarf galaxies in different environments
• Distribution of Singularities in the Cosmic Microwave Background Polarization
• Cross-Correlation Studies between CMB Temperature Anisotropies and 21 cm Fluctuations
• The Stellar Initial Mass Function at the Epoch of Reionization
• Ultraviolet modified photons and anisotropies in the cosmic microwave background radiation
• Brane inflation driven by noncanonical scalar field
• Was the Universe Reionized at Redshift 10?
• Clues to AGN Growth from Optically Variable Objects in the Hubble Ultra Deep Field
• Beam mismatch effects in Cosmic Microwave Background polarization measurements
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Observations of HI 21cm absorption by the neutral IGM during the epoch of re-ionization with the Square Kilometer Array
• Degenerate sterile neutrino dark matter in the cores of galaxies
• Large-Scale Non-Gaussianities in the 21 cm Background Anisotropies From the Era of Reionization
• Distinguishing standard reionization from dark matter models
• Dynamical system analysis in teleparallel gravity with boundary term
• A Faraday Rotation Template for the Galactic Sky
• Cosmology with the CMB temperature-polarization correlation
• Constraints on alternative models to dark energy
• Do Observations Favour Galileon Over Quintessence?
• Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?
• The Cosmic Near Infrared Background III: Fluctuations, Reionization and the Effects of Minimum Mass and Self-regulation
• Quadratic estimator for CMB cross-correlation
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• Constraining Cut-off Physics in the Cosmic Microwave Background
• The Sky Polarization Observatory
• Disappearing Dark Matter in Brane World Cosmology: New Limits on Noncompact Extra Dimensions
• Reionization in the Warm Dark Matter Model
• An improved upper limit to the CMB circular polarization at large angular scales
• Collision of Domain Walls in asymptotically Anti de Sitter spacetime
• Boundary Inflation and the WMAP Data
• Single Field Inflation models allowed and ruled out by the three years WMAP data
• Trans-Planckian corrections to the primordial spectrum in the infra-red and the ultra-violet
• Ionizing radiation from hydrogen recombination strongly suppresses the lithium scattering signature in the CMB
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• An Interacting model of Dark Energy in Brans-Dicke theory
• Planck intermediate results. XLIX. Parity-violation constraints from polarization data
• Tracking quintessence: a dynamical systems study
• Cosmic Superstrings and Primordial Magnetogenesis
• Radiation from early black holes - I: effects on the neutral inter-galactic medium
• Cosmic Renaissance: The First Sources of Light
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Systematic Errors in Cosmic Microwave Background Interferometry
• Observational Constraints on Dynamical Dark Energy Models
• On Minkowski Functionals of CMB polarization
• Searching for Primordial Magnetic Fields with CMB B-modes
• The CMB Quadrupole in a Polarized Light
• History of Hydrogen Reionization in the Cold Dark Matter Model
• CMBfit: Rapid WMAP likelihood calculations with normal parameters
• Testing generalized logotropic models with cosmic growth
• Consistency equations in Randall-Sundrum cosmology: a test for braneworld inflation
• Cosmic infrared background from Population III stars and its effect on spectra of high-z gamma-ray bursts
• The reionization of galactic satellite populations
• CMB EB and TB cross-spectrum estimation via pseudo-spectrum techniques
• High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair
• Stochastic Quintessence
• Polarization of 21cm Radiation from the Epoch of Reionization
• The Galactic globular cluster system as a fossil record of reionization
• Tangled magnetic fields and CMBR signal from reionization epoch
• Physics of the cosmic microwave background anisotropy
• Neutrino Signatures from the First Stars
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• The cosmological evolution of metal enrichment in quasar host galaxies
• CMB power spectrum estimation using noncircular beams
• Neutrino number asymmetry and cosmological birefringence
• Detecting Reionization in the Star Formation Histories of High-Redshift Galaxies
• Cosmic acceleration and extra dimensions: constraints on modifications of the Friedmann equation
• Star Forming Galaxies at z~6 and Reionization
• Self-interacting Scalar Field Trapped in a Randall-Sundrum Braneworld: The Dynamical Systems Perspective
• COMPASS: An Upper Limit on CMB Polarization at an Angular Scale of 20 arc minutes
• Unified Models of Inflation and Quintessence
• Scaling defect decay and the reionization history of the Universe
• Transition From Population III to Population II Stars
• Gravitational-wave background from compact objects embedded in AGN accretion disks
• UHE neutrinos from Pop III stars: concept and constraints
• The Standard Cosmological Model
• Constraints on Star Forming Galaxies at z> 6.5 from HAWK-I Y-band Imaging of GOODS-South
• The Formation and Evolution of the First Massive Black Holes
• Fossil records of cosmic reionization in galactic stellar halos
• Hints of star fomation at z>6: the chemical abundances of the DLA system in the QSO BRI 1202-0725 (z_abs = 4.383)
• Generalised scalar-tensor theory and the cosmic acceleration
• CMB-induced Cluster Polarization as a Cosmological Probe
• Antenna Instrumental Polarization and its Effects on E- and B-Modes for CMBP Observations
• Separating polarized cosmological and galactic emissions for CMB B-mode polarization experiments
• Modified theory of gravity and the history of cosmic evolution
• On the Origin of Mass--Metallicity Relations, Blue Tilts, and Scaling Relations for Metal-poor Globular Cluster Systems
• Primordial non-Gaussian signatures in CMB polarization
• Gemini H-band imaging of the field of a z=10 candidate
• Boosting hierarchical structure formation with scalar-interacting dark matter
• Imprint of Inhomogeneous Reionization on the Power Spectrum of Galaxy Surveys at High Redshifts
• A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism
• Reconstructing large running-index inflaton potentials
• Magneto-optic effects of the Cosmic Microwave Background
• Gemini-South + FLAMINGOS Demonstration Science: Near-Infrared Spectroscopy of the z=5.77 Quasar SDSS J083643.85+005453.3
• Have we detected one of the sources responsible for an early reionisation of the Universe?
• Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion
• MAXIPOL: A Balloon-borne Experiment for Measuring the Polarization Anisotropy of the Cosmic Microwave Background Radiation
• The Infrared Glow of First Stars
• New constraint on the cosmological background of relativistic particles
• Early reionization by cosmic strings revisited
• Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
• Exploring two-spin internal linear combinations for the recovery of the CMB polarization
• Constraining the epoch of reionization from the observed properties of the high-z Universe
• A polarized synchrotron template for CMBP experiments after WMAP data
• Triggering the Formation of Halo Globular Clusters with Galaxy Outflows
• Quasars as Probes of Late Reionization and Early Structure Formation
• Gravitational waves in the generalized Chaplygin gas model
• An analytic model for the transition from decelerated to accelerated cosmic expansion
• Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Curvaton Scenario with Affleck-Dine Baryogenesis
• Trade-off between angular resolution and straylight contamination in CMB anisotropy experiments. II. Straylight evaluation
• POKER: Estimating the power spectrum of diffuse emission with complex masks and at high angular resolution
• The conventions for the polarization angle
• Polarization Signals of the 21 cm Background from the Era of Reionization
• Measuring CMB Polarization with BOOMERANG
• Primordial quadrupole-induced polarisation from filamentary structures and galaxy clusters
• Late-end reionization with ATON-HE: towards constraints from Lyman-$\alpha$ emitters observed with JWST
• The Integrated Sachs-Wolfe effect as a probe of non-standard cosmological evolution
• Primordial Gravitational Waves and Inflation: CMB and Direct Detection With Space-Based Laser Interferometers
• Searching for the Sources Responsible for Cosmic Reionization: Probing 7 < z < 10 and Beyond
• Near-Infrared Colors of Gamma-Ray Burst Afterglows and Cosmic Reionization History
• Galaxies Inside Stromgren Spheres of Luminous Quasars at z>6: Detection of The First Galaxies
• Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data
• Cosmic Chemical Evolution with an Early Population of Intermediate Mass Stars
• Early reionization by decaying particles and cosmic microwave background radiation
• Cosmic microwave background polarization analysis
• E/B Separation in CMB Interferometry
• Imprint of Gravitational Lensing by Population III Stars in Gamma Ray Burst Light Curves
• Evidence for new physics from clusters ?
• Observational Cosmology
• Observations of the High Redshift Universe
• CMB Anisotropy Due to Tangled magnetic fields in re-ionized models
• Data analysis methods for the cosmic microwave background
• Spectral Spatial Fluctuations of CMBR: Strategy and Concept of the Experiment
• Searching For Integrated Sachs-Wolfe Effect Beyond Temperature Anisotropies: CMB E-mode Polarization-Galaxy Cross Correlation
• Reanalysis of the spectrum of the z=10 galaxy
• Limits on the Polarization of the Cosmic Microwave Background Radiation at Multipoles up to l~2000
• Cosmic reionization by primordial cosmic rays
• Small scale contributions to CMB: A coherent analysis
• A model for CMB anisotropies on large angular scales
• Modular thermal inflation without slow-roll approximation
• Implications of the Lyman alpha Emission Line from a Candidate z=10 Galaxy
• Falsifying Field-based Dark Energy Models
• Could the next generation of cosmology experiments exclude supergravity?
• The influence of ultra-high-energy cosmic rays on star formation in the early universe
• On the Effects due to a Decaying Cosmological Fluctuation
• Wide Field Surveys and Astronomical Discovery Space
• Suppression of Dwarf Galaxy Formation by Cosmic Shocks
• Milli-charged fermion vacuum polarization in cosmic magnetic fields and generation of CMB elliptic polarization
• A 77-118 GHz Resonance-free Septum Polarizer
• Probing galaxy density profiles with future supernova surveys
• Quintessence and the Curvature of the Universe after WMAP
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Light mass galileon and late time acceleration of the Universe
• Did Galaxy Assembly and Supermassive Black-Hole Growth go hand-in-hand?
• Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy
• Site Evaluation and RFI spectrum measurements in Portugal at the frequency range 0.408-10 GHz for a GEM polarized galactic radio emission experiment
• On the CMB circular polarization. I. The Cotton-Mouton effect
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Study of a Neutrino Mass Texture Generated in Supergravity with Bilinear R-Parity Violation
• The current status of observational cosmology
• Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Radio views of cosmic reionization
• Observational Constraints on Axions as Quintessence in String Theory
• Discriminating neutrino mass models using Type II seesaw formula
• Sunyaev-Zeldovich effects, free-free emission, and imprints on the cosmic microwave background
• The optimal redshift for detecting ionized bubbles in HI 21-cm maps
• Effect of the length of inflation on angular TT and TE power spectra in power-law inflation
• Late-time acceleration with steep exponential potentials
• CMB power spectrum estimation with non-circular beam and incomplete sky coverage
• Oxygen pumping II: Probing the Inhomogeneous Metal Enrichment at the Epoch of Reionization with High Frequency CMB Observations
• Inflation on Fractional Branes: D--Brane Inflation as D--Term Inflation
• Lyman Break Galaxies and Reionization of the Universe
• Predictions of mixed non-Gaussian cosmological density fields for the cosmic microwave background radiation
• Statistical characteristics of observed Ly-$\alpha$ forest and the shape of linear power spectrum
• New Quantum Phase of the Universe before Inflation and its Cosmological and Dark Energy Implications
• CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
• Low-frequency line temperatures of the CMB
• CMB Optical Depth Measurements: Past, Present, Future
• Non-Minimal Quintessence With Nearly Flat Potential
• Can neutrino viscosity drive the late time cosmic acceleration?
• The early phases of Milky Way's chemical evolution
• Statistical characteristics of observed Ly-$\alpha$ forest and the shape of initial power spectrum
• Quark-Novae, cosmic reionization, and early r-process element production
• Non-Circular beam correction to the CMB power spectrum
• Early reionization by decaying particles in the light of three year WMAP data
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• CMB Polarization as complementary information to anisotropies
• Dust during the Reionization
• Cross-Correlation Studies with CMB Polarization Maps
• Isocurvature Fluctuations Induce Early Star Formation
• The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra
• Full-sky correlation functions for CMB experiments with asymmetric window functions
• Cosmic Microwave Background Polarization and reionization: constraining models with a double reionization
• First Results from the Arcminute Cosmology Bolometer Array Receiver
• Plasma Suppression of Large Scale Structure Formation in the Universe
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Formation of First Stars Triggered by Collisions and Shockwaves: Prospect for High Star Formation Efficiency and High Ionizing Photon Escape Fraction
• Statistical features of 21-cm emission from the epoch between reionization and Gunn-Peterson transparency
• On the Origin of the Kinematical Differences Between the Stellar Halo and the Old Globular Cluster System in the Large Magellanic Cloud
• A Far Infrared Polarimeter
• New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3
• Dynamic domain walls in Maxwell-Dilaton background
• Domain walls in Born-Infeld-dilaton background
• Gravitational Field of a Spinning Cosmic String
• Slow-roll inflationary senario in the maximally extended background
• Propagating spatially-varying multiplicative shear bias to cosmological parameter estimation for stage-IV weak-lensing surveys
• Density perturbations from both the inflaton and the curvaton
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Deep VLT V-band Imaging of the Field of a z=10 Candidate Galaxy: Below the Lyman Limit?
• Constraining the reionization history with large angle CMB polarization
• Semiclassical (Quantum Field Theory) and Quantum (String) de Sitter Regimes: New Results
• Spectra from Forming Region of the First Galaxies : The Effect of Aspherical Deceleration
• Quantum Trans-Planckian Physics inside Black Holes and its Spectrum
• Optical and Infrared Non-detection of the z=10 Galaxy Behind Abell 1835
• The Effect of Lensing on the Large-Scale CMB Anisotropy
• The T-E correlation coefficient of Planck legacy data
• On the wavelet analysis of CMB time ordered data: application to Archeops
• Cosmic reionization constraints on the nature of cosmological perturbations
• Lyman Alpha Line Spectra of the First Galaxies: Dependence on Observed Direction to the Underlying CDM Filament
• A very extended reionization epoch ?
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• Polarization experiments
• First Stars. I. Evolution without mass loss
• First Light and Reionization: A Conference Summary
• Coherent states of quantum spacetimes for black holes and de Sitter spacetime
• Status and Perspectives of Neutrino Physics
• Modeling the accretion history of supermassive black holes
• Cross-Correlation Detection of Point Sources in WMAP First Year Data
• Foreground removal from WMAP 7yr polarization maps using an MLP neural network
• The synchrotron foreground and CMB temperature-polarization cross correlation power spectrum from the first year WMAP data
• Particle Physics and the Cosmic Microwave Background
• Are There Any Redshift >8 Gamma-Ray Bursts in the BATSE Catalog?
• Problems with the Current Cosmological Paradigm
• Reconstructing the epoch of reionisation with Planck PR4
• Entropy Production in the Inflationary Epoch Using the Gouy-Stodola Theorem
• Perspectives on fundamental cosmology from Low Earth Orbit and the Moon
• Inhomogeneous structure formation may alleviate need for accelerating universe
• CMB B-mode polarization from Thomson scattering in the local universe
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Cosmic Microwave Background Polarization
• Metal Enrichment of the Intergalactic Medium and Production of Massive Black Holes
• Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
• Spatial Correlation of Massive Black Hole Mergers: Probing the Formation Mechanism and Reionization
• A model of inflation independent of the initial conditions, with bounded number of e-folds and n_s larger orsmaller than one
• Predicting the Polarization of The Microwave Background from the WMAP Temperature Maps
• The CAPMAP Instrument and its First Season
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• The Cosmic Microwave Background anisotropies: open problems
• The Classical and Quantum Inflaton: the Precise Inflationary Potential and Quantum Inflaton Decay after WMAP
• Combined $13\times 2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints
• Application of beam deconvolution technique to power spectrum estimation for CMB measurements
• Clarifying Inflation Models: the Precise Inflationary Potential from Effective Field Theory and the WMAP data
• Linking radio to infrared: a radio source count model
• The Reionization History in the Lognormal Model
• Semiclassical and Quantum Black Holes and their Evaporation, de Sitter and Anti-de Sitter Regimes, Gravitational and String Phase Transitions
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Cosmology with CMB anisotropy
• Pico: Parameters for the Impatient Cosmologist
• Effects of Thermal Fluctuations in the SPOrt Experiment
• A new approach to modified-gravity models
• Angular Power Spectrum in Modular Invariant Inflation Model
• The Ku-band Polarization Identifier
• Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• Constraining Planck scale physics with CMB and Reionization Optical Depth
• Statistical Imprints of SZ Effects in the Cosmic Microwave Background
• Maps of the Cosmos: The Cosmic Microwave Background
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Influence of Plasma Collective Effects on Cosmological Evolution
• Summary of ICGC04 Cosmology Workshop
• `Standard' Cosmological model & beyond with CMB
• Close Pairs as Probes of the Galaxy's Chemical Evolution
• Do We Live in a Vanilla Universe? Theoretical Perspectives on WMAP
• The Relic Neutrino Backround from the First Stars
• From z>6 to z~2: Unearthing Galaxies at the Edge of the Dark Ages
• Cosmological quests in the CMB sky
• A survey of NB921 dropouts in the Subaru Deep Field