A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
arXiv:0803.2157 · doi:10.1111/j.1365-2966.2008.13406.x
Abstract
We repeat the directional spherical real Morlet wavelet analysis, used to detect non-Gaussianity in the Wilkinson Microwave Anisotropy Probe (WMAP) 1-year and 3-year data (McEwen et al. 2005, 2006a), on the WMAP 5-year data. The non-Gaussian signal detected previously is present in the 5-year data at a slightly increased statistical significance of approximately 99%. Localised regions that contribute most strongly to the non-Gaussian signal are found to be very similar to those detected in the previous releases of the WMAP data. When the localised regions detected in the 5-year data are excluded from the analysis the non-Gaussian signal is eliminated.
4 pages, 4 figures, replaced to match version accepted by MNRAS, masks available for download
References in corpus (57)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
- The significance of the largest scale CMB fluctuations in WMAP
- Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets
- The axis of evil
- Is the low-l microwave background cosmic?
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
- Multipole Vectors--a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2<=l<=8
- Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps
- On the large-angle anomalies of the microwave sky
- On Foreground Removal from the Wilkinson Microwave Anisotropy Probe Data by an Internal Linear Combination Method: Limitations and Implications
- Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
- The non-Gaussian Cold Spot in the 3-year WMAP data
- Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton
- The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution
- Asymmetries in the local curvature of the WMAP data
- Non-Gaussianity of the derived maps from the first-year WMAP data
- Limits on f_NL parameters from WMAP 3yr data
- A high-significance detection of non-Gaussianity in the WMAP 1-year data using directional spherical wavelets
- Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
- Is the Universe odd?
- The Hot and Cold Spots in the WMAP Data are Not Hot and Cold Enough
- Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data
- Fast Convolution on the Sphere
- Wavelets and WMAP non-Gaussianity
- Correspondence principle between spherical and Euclidean wavelets
- Phase Correlations in Cosmic Microwave Background Temperature Maps
- Assessing the effects of foregrounds and sky removal in WMAP
- The N-point correlation functions of the first-year Wilkinson Microwave Anisotropy Probe sky maps
- Point Source Detection using the Spherical Mexican Hat Wavelet on simulated all-sky Planck maps
- Global universe anisotropy probed by the alignment of structures in the cosmic microwave background
- Fast directional continuous spherical wavelet transform algorithms
- A high-significance detection of non-Gaussianity in the WMAP 3-year data using directional spherical wavelets
- A low CMB variance in the WMAP data
- The Multipole Vectors of WMAP, and their frames and invariants
- 3-point temperature anisotropies in WMAP: Limits on CMB non-Gaussianities and non-linearities
- Testing Gaussian random hypothesis with the cosmic microwave background temperature anisotropies in the three-year WMAP data
- Non-Gaussianity detections in the Bianchi VIIh corrected WMAP 1-year data made with directional spherical wavelets
- A Scaling Index Analysis of the WMAP three year data: Signatures of non-Gaussianities and Asymmetries in the CMB
- Primordial non-Gaussianity: local curvature method and statistical significance of constraints on f_NL from WMAP data
- Genus Topology of the Cosmic Microwave Background from WMAP
- Non-Gaussianity in the WMAP data using the peak-peak correlation function
- Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
- Non-Random Phases in Non-Trivial Topologies
- Deviation from Gaussianity in the cosmic microwave background temperature fluctuations
- Non-Gaussianity analysis on local morphological measures of WMAP data
- Measuring the Three Point Correlation Function of the Cosmic Microwave Background
- Auto and cross correlation of phases of the whole-sky CMB and foreground maps from the 1-year WMAP data
- On the bispectrum of COBE and WMAP
- Non-Gaussian Foreground Residuals of the WMAP First Year Maps
- Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
- Probing Non-Gaussianity In The Cosmic Microwave Background Anisotropies: One Point Distribution Function
Cited by in corpus (56)
- Increasing evidence for hemispherical power asymmetry in the five-year WMAP data
- Spherical Needlets for CMB Data Analysis
- Volume Modulus Inflation and the Gravitino Mass Problem
- Signature of Primordial Non-Gaussianity on Matter Power Spectrum
- Primordial Non-Gaussianities of General Multiple Field Inflation
- Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations
- Tests and problems of the standard model in Cosmology
- Fast directional continuous spherical wavelet transform algorithms
- Cosmological applications of a wavelet analysis on the sphere
- A low CMB variance in the WMAP data
- Non-Gaussian Inflationary Perturbations from the dS/CFT Correspondence
- Isotropy of the early universe from CMB anisotropies
- Exact Wavelets on the Ball
- Markov chain Monte Carlo analysis of Bianchi VII_h models
- Constraints on Primordial Non-Gaussianity from a Needlet Analysis of the WMAP-5 Data
- Anomalous CMB north-south asymmetry
- Localisation of directional scale-discretised wavelets on the sphere
- Halo abundances in the f_{nl} model
- Complex data processing: fast wavelet analysis on the sphere
- A model-independent test for scale-dependent non-Gaussianities in the CMB
- Needlet Bispectrum Asymmetries in the WMAP 5-year Data
- Long range correlation in cosmic microwave background radiation
- The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
- Second-Generation Curvelets on the Sphere
- A Theory of a Spot
- Non-Gaussianity analysis on local morphological measures of WMAP data
- Directional spin wavelets on the sphere
- Non-Gaussian Signatures in the five-year WMAP data as identified with isotropic scaling indices
- Wavelet-Bayesian inference of cosmic strings embedded in the cosmic microwave background
- Searching for non-Gaussianity in the WMAP data
- Non-gaussianity in the foreground-reduced CMB maps
- Is the cold spot responsible for the CMB North-South asymmetry?
- Too few spots in the cosmic microwave background
- The One-dimensional Fourier Representation and Large Angular Scale Foreground Contamination in the 3-year Wilkinson Microwave Anisotropy Probe data
- Peaks in the CMBR power spectrum. II. Physical interpretation for any cosmological scenario
- Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
- The nonlinear probability distribution function in models with local primordial non-Gaussianity
- Fast Calculation of the Weak Lensing Aperture Mass Statistic
- Scale-dependent non-Gaussianities in the WMAP data as identified by using surrogates and scaling indices
- Foreground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year data
- Phase analysis of the cosmic microwave background from an incomplete sky coverage
- Wilkinson Microwave Anisotropy Probe 7-yr constraints on fNL with a fast wavelet estimator
- Impact of the 1/f noise and the asymmetric beam on non-Gaussianity searches with Planck
- The pairwise velocity probability density function in models with local primordial non-Gaussianity
- Cosmic microwave background anomalies viewed via Gumbel Statistics
- The nonlinear redshift space probability distribution function in models with local primordial non-Gaussianity
- Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
- Search for non-Gaussianities in the WMAP data with the Scaling Index Method
- Using spherical wavelets to search for magnetically-induced alignment in the arrival directions of ultra-high energy cosmic rays
- Constraining Modified Gravity with Large non-Gaussianities
- Constraints on fNL from Wilkinson Microwave Anisotropy Probe 7-year data using a neural network classifier
- Non-Gaussianity in the HILC foreground-reduced three-year WMAP CMB map
- A Study of Gaussianity in CMB band maps
- Improved Method for Detecting Local Discontinuities in CMB data by Finite Differencing
- Scale-discretised ridgelet transform on the sphere
- Investigating non-Gaussianity in Cosmic Microwave Background Temperature Maps using Spherical Harmonic Phases