Phase cross-correlation of the WMAP ILC map and foregrounds
arXiv:astro-ph/0310542 · doi:10.1086/381249
Abstract
We present a circular cross-correlation tests for the phases of the Internal Linear Combination Map (ILC) and {\it WMAP}'s foregrounds for all K--W frequency bands at the range of multipoles . We have found significant deviations from the expected Poissonian statistics for the ILC and the foregrounds phases. Our analysis shows that the low multipole range of the ILC power spectrum contains some of the foregrounds residues.
4 pages, 3 figures. Submitted to ApJL
References in corpus (13)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- A Line of Sight Approach to Cosmic Microwave Background Anisotropies
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
- The Microwave Anisotropy Probe (MAP) Mission
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits
- Non-Gaussianity of the derived maps from the first-year WMAP data
- Phase Information and the Evolution of Cosmological Density Perturbations
- Return mapping of phases and the analysis of the gravitational clustering hierarchy
- Genus Topology of the Cosmic Microwave Background from WMAP
- Phase Correlations in Non-Gaussian Fields
- Combined multi-frequency map for point source substraction
Cited by in corpus (33)
- Testing the cosmological principle of isotropy: local power spectrum estimates of the WMAP data
- Asymmetries in the local curvature of the WMAP data
- Gauss--Legendre Sky Pixelization (GLESP) for CMB maps
- Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data
- A Hint of Poincaré Dodecahedral Topology in the WMAP First Year Sky Map
- Statistical Isotropy of the Wilkinson Microwave Anisotropy Probe Data: A Bipolar Power Spectrum Analysis
- Primordial magnetic field and non-Gaussianity of the 1-year Wilkinson Microwave Anisotropy Probe (WMAP) data
- Testing Gaussian random hypothesis with the cosmic microwave background temperature anisotropies in the three-year WMAP data
- The Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Errors due to pixelization of the CMB sky
- Statistics of phase correlations as a test for non-Gaussianity of the CMB maps
- Cosmological parameters and the WMAP data revisited
- A Faraday Rotation Template for the Galactic Sky
- Instability of reconstruction of the low CMB multipoles
- Pearson's random walk in the space of the CMB phases: evidence for parity asymmetry
- Random-Walk Statistics and the Spherical Harmonic Representation of CMB Maps
- Can residuals of the Solar system foreground explain low multipole anomalies of the CMB ?
- The One-dimensional Fourier Representation and Large Angular Scale Foreground Contamination in the 3-year Wilkinson Microwave Anisotropy Probe data
- Tessellated Mapping of Cosmic Background Radiation Correlations and Source Distributions
- Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches
- Auto and cross correlation of phases of the whole-sky CMB and foreground maps from the 1-year WMAP data
- Dominant Multipoles in WMAP5 Mosaic Data Correlation Maps
- Foreground analysis from the 1-year Wilkinson Microwave Anisotropy Probe (WMAP) data
- Peculiarities of phases of the WMAP quadrupole
- Correlations from Galactic foregrounds in the 1-year Wilkinson Microwave Anisotropy Probe WMAP data
- Cosmic crystallography using short-lived objects - active galactic nuclei
- Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
- Symmetry of the CMB sky as a new test of its statistical isotropy. Non Cosmological Octupole?
- Statistical properties of polarized CMB foreground maps
- Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
- Correlation properties of the maps of the NVSS survey and WMAP ILC
- The synchrotron foreground and CMB temperature-polarization cross correlation power spectrum from the first year WMAP data
- Structure in Galaxy Distribution. III. Fourier Transforming the Universe
- Cosmic Microwave Background anisotropies: the power spectrum and beyond