Optimal and fast E/B separation with a dual messenger field
arXiv:1801.05358 · doi:10.1093/mnras/sty341
Abstract
We adapt our recently proposed dual messenger algorithm for spin field reconstruction and showcase its efficiency and effectiveness in Wiener filtering polarized cosmic microwave background (CMB) maps. Unlike conventional preconditioned conjugate gradient (PCG) solvers, our preconditioner-free technique can deal with high-resolution joint temperature and polarization maps with inhomogeneous noise distributions and arbitrary mask geometries with relative ease. Various convergence diagnostics illustrate the high quality of the dual messenger reconstruction. In contrast, the PCG implementation fails to converge to a reasonable solution for the specific problem considered. The implementation of the dual messenger method is straightforward and guarantees numerical stability and convergence. We show how the algorithm can be modified to generate fluctuation maps, which, combined with the Wiener filter solution, yield unbiased constrained signal realizations, consistent with observed data. This algorithm presents a pathway to exact global analyses of high-resolution and high-sensitivity CMB data for a statistically optimal separation of E and B modes. It is therefore relevant for current and next-generation CMB experiments, in the quest for the elusive primordial B-mode signal.
arXiv comment11 pages, 5 figures, 1 table. Accepted for publication in MNRAS main journal
References in corpus (68)
- Planck 2015 results. XIII. Cosmological parameters
- Efficient Computation of CMB anisotropies in closed FRW models
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- An All-Sky Analysis of Polarization in the Microwave Background
- Statistics of Cosmic Microwave Background Polarization
- Signature of Gravity Waves in Polarization of the Microwave Background
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- A Probe of Primordial Gravity Waves and Vorticity
- Cosmic Microwave Background Anisotropies
- A CMB Polarization Primer
- Estimating the Power Spectrum of the Cosmic Microwave Background
- How to measure CMB power spectra without losing information
- The Quest for B Modes from Inflationary Gravitational Waves
- Detection of Gravitational Lensing in the Cosmic Microwave Background
- Reconstruction of lensing from the cosmic microwave background polarization
- Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
- Measuring primordial non-Gaussianity in the cosmic microwave background
- Gravitational lensing as a contaminant of the gravity wave signal in CMB
- How to make maps from CMB data without losing information
- Global, Exact Cosmic Microwave Background Data Analysis Using Gibbs Sampling
- Power spectrum estimation from high-resolution maps by Gibbs sampling
- Analysis of CMB polarization on an incomplete sky
- E/B decomposition of finite pixelized CMB maps
- An Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps
- Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background
- Bayesian power-spectrum inference for Large Scale Structure data
- Pseudo- estimators which do not mix E and B modes
- CMB Polarization can constrain cosmology better than CMB temperature
- Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach
- A general solution to the E-B mixing problem
- De-contamination of cosmological 21-cm maps
- The nature of the E-B decomposition of CMB polarization
- Cross-correlation of CMB with large-scale structure: weak gravitational lensing
- Hierarchical Cosmic Shear Power Spectrum Inference
- Error analysis of quadratic power spectrum estimates for CMB polarization: sampling covariance
- Bayesian Power Spectrum Analysis of the First-Year WMAP data
- Improved simulation of non-Gaussian temperature and polarization CMB maps
- Estimation of Polarized Power Spectra by Gibbs sampling
- CMB Polarization B-mode Delensing with SPTpol and Herschel
- Efficient Wiener filtering without preconditioning
- Bayesian delensing of CMB temperature and polarization
- CMB Temperature and Polarization Anisotropy Fundamentals
- Methods for Bayesian power spectrum inference with galaxy surveys
- Wiener Filtering of the COBE DMR Data
- Harmonic E/B decomposition for CMB polarization maps
- Bayesian 3d velocity field reconstruction with VIRBIuS
- Separating E and B types of polarization on an incomplete sky
- Bayesian inference of CMB gravitational lensing
- CMB E/B decomposition of incomplete sky: a pixel space approach
- Detectability of Microwave Background Polarization
- Matrix-free Large Scale Bayesian inference in cosmology
- How to make a clean separation between CMB E and B modes with proper foreground masking
- Efficient decomposition of cosmic microwave background polarization maps into pure E, pure B, and ambiguous components
- Pure pseudo-C_l estimators for CMB B-modes
- Multi-resolution Bayesian CMB component separation through Wiener-filtering with a pseudo-inverse preconditioner
- Wiener filter reloaded: fast signal reconstruction without preconditioning
- Wavelet reconstruction of E and B modes for CMB polarisation and cosmic shear analyses
- Local non-Gaussianity in the Cosmic Microwave Background the Bayesian way
- Pure E and B polarization maps via Wiener filtering
- Bayesian power-spectrum inference with foreground and target contamination treatment
- Spin-SILC: CMB polarisation component separation with spin wavelets
- A wavelet-Galerkin algorithm of the E/B decomposition of CMB polarization maps
- A multi-level solver for Gaussian constrained CMB realizations
- Likelihood, Fisher information, and systematics of cosmic microwave background experiments
- Fast calculation of the Fisher matrix for cosmic microwave background experiments
- Cosmic Microwave Background Mapmaking with a Messenger Field
- MasQU: Finite Differences on Masked Irregular Stokes Q,U Grids
- Preconditioner-free Wiener filtering with a dense noise matrix
Cited by in corpus (7)
- Wiener filtering and pure E/B decomposition of CMB maps with anisotropic correlated noise
- Fingerprint of Galactic Loop I on polarized microwave foregrounds
- Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
- B-mode Power Spectrum of CMB via Polarized Compton Scattering
- Testing Quadratic Maximum Likelihood estimators for forthcoming Stage-IV weak lensing surveys
- From top-hat masking to smooth transitions: P-filter and its application to polarized microwave sky maps
- Reconstruction of full sky CMB and modes spectra removing -to- leakage from partial sky using deep learning