Hybrid estimation of cosmic microwave background polarization power spectra
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Open Access
- 17 July 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 370 (1) , 343-362
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This publication has 36 references indexed in Scilit:
- Detectability of tensor modes in the presence of foregroundsPhysical Review D, 2005
- Cosmic microwave background temperature and polarization pseudo-Cℓestimators and covariancesMonthly Notices of the Royal Astronomical Society, 2005
- Error analysis of quadratic power spectrum estimates for cosmic microwave background polarization: sampling covarianceMonthly Notices of the Royal Astronomical Society, 2005
- Separating E from BNew Astronomy Reviews, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Foreground EmissionThe Astrophysical Journal Supplement Series, 2003
- E/Bdecomposition of finite pixelized CMB mapsPhysical Review D, 2003
- All-sky convolution for polarimetry experimentsPhysical Review D, 2000
- Computing challenges of the cosmic microwave backgroundComputing in Science & Engineering, 1999
- Estimating the power spectrum of the cosmic microwave backgroundPhysical Review D, 1998