Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
arXiv:astro-ph/0511550 · doi:10.1086/499804
Abstract
We cross correlate the Wilkinson Microwave Anisotropy Probe (WMAP) first year data and the diffuse gamma-ray intensity maps from the Energetic Gamma Ray Experiment Telescope (EGRET) using spherical wavelet approaches. Correlations at 99.7% significance level have been detected, at scales around in the WMAP foreground cleaned W-band and Q-band maps, based on data from regions that are outside the most conservative WMAP foreground mask; no significant correlation is found with the Tegmark cleaned map. The detected correlation is most likely of Galactic origin, and thus can help us probing the origins of possible Galactic foreground residuals and ultimately removing them from measured microwave sky maps.
4 pages, 7 figures; accepted for publication in ApJL
References in corpus (38)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
- Diffuse continuum gamma rays from the Galaxy
- A high resolution foreground cleaned CMB map from WMAP
- Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS
- A Full-Sky H-alpha Template for Microwave Foreground Prediction
- Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets
- A correlation of the cosmic microwave sky with large scale structure
- A method for subtracting foregrounds from multi-frequency CMB sky maps
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
- 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
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources
- Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton
- Asymmetries in the local curvature of the WMAP data
- Non-Gaussianity of the derived maps from the first-year WMAP data
- Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
- Cross-correlation of the CMB and radio galaxies in real, harmonic and wavelet spaces: detection of the integrated Sachs-Wolfe effect and dark energy constraints
- A high-significance detection of non-Gaussianity in the WMAP 1-year data using directional spherical wavelets
- The performance of spherical wavelets to detect non-Gaussianity in the CMB sky
- Wavelets and WMAP non-Gaussianity
- Correspondence principle between spherical and Euclidean wavelets
- Wavelet analysis and the detection of non-Gaussianity in the CMB
- Testing the Gaussianity of the COBE-DMR data with spherical wavelets
- Spherical Mexican Hat wavelet: an application to detect non-Gaussianity in the COBE-DMR maps
- Cross-Correlation of the Cosmic Microwave Background with Radio Sources: Constraints on an Accelerating Universe
- Phase cross-correlation of the WMAP ILC map and foregrounds
- COBE-DMR constraints on the nonlinear coupling parameter: a wavelet based method
- Cross-correlation of the CMB and foregrounds phases derived from the WMAP data
- Non-Gaussianity: Comparing wavelet and Fourier based methods
- Evidence for Dark Matter Annihilation from Galactic Gamma Rays?
- The large-scale polarization of the microwave background and foreground
- Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches
- Foreground contributions to the Cosmic Microwave Background
- Simulations of the Microwave Sky and of its ``Observations''
Cited by in corpus (9)
- 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
- Tests and problems of the standard model in Cosmology
- A comprehensive overview of the Cold Spot
- Optimal ISW detection and joint likelihood for cosmological parameter estimation
- High Galactic Latitude Interstellar Neutral Hydrogen Structure and Associated (WMAP) High Frequency Continuum Emission
- Wavelet-based cross-correlation analysis of structure scaling in turbulent clouds
- Some doubts on the validity of the foreground Galactic contribution subtraction from microwave anisotropies
- Correlation Analysis between Tibet AS- TeV Cosmic Ray and WMAP Nine-year Data