Likelihood techniques for the combined analysis of CMB temperature and polarization power spectra
Open Access
- 29 September 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 372 (3) , 1104-1116
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This publication has 22 references indexed in Scilit:
- 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
- HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the SphereThe Astrophysical Journal, 2005
- Myths and truths concerning estimation of power spectra: the case for a hybrid estimatorMonthly Notices of the Royal Astronomical Society, 2004
- A maximum likelihood analysis of the low cosmic microwave background multipoles from theWilkinson Microwave Anisotropy ProbeMonthly Notices of the Royal Astronomical Society, 2004
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- Analytic marginalization over CMB calibration and beam uncertaintyMonthly Notices of the Royal Astronomical Society, 2002
- Radical Compression of Cosmic Microwave Background DataThe Astrophysical Journal, 2000
- Cosmic Complementarity: Joint Parameter Estimation from Cosmic Microwave Background Experiments and Redshift SurveysThe Astrophysical Journal, 1999
- Estimating the power spectrum of the cosmic microwave backgroundPhysical Review D, 1998