Template fitting and the large-angle cosmic microwave background anomalies
Open Access
- 14 March 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 367 (4) , 1714-1720
- https://doi.org/10.1111/j.1365-2966.2006.10078.x
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- Topological signatures in CMB temperature anisotropy mapsPhysical Review D, 2005
- Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA‐I FieldThe Astrophysical Journal, 2004
- Assessing the effects of foregrounds and sky removal in WMAPPhysical Review D, 2004
- A hint of Poincaré dodecahedral topology in the WMAP first year sky mapAstronomy & Astrophysics, 2004
- Detection of Non‐Gaussianity in theWilkinson Microwave Anisotropy ProbeFirst‐Year Data Using Spherical WaveletsThe Astrophysical Journal, 2004
- Exact likelihood evaluations and foreground marginalization in low resolution WMAP dataPhysical Review D, 2004
- Asymmetries in the Cosmic Microwave Background Anisotropy FieldThe Astrophysical Journal, 2004
- Significance of the largest scale CMB fluctuations in WMAPPhysical Review D, 2004
- Limits to global rotation and shear from the COBE DMR four-year sky mapsPhysical Review D, 1997
- How Anisotropic is Our Universe?Physical Review Letters, 1996