Maximum Likelihood algorithm for parametric component separation in CMB experiments
arXiv:0804.2645 · doi:10.1111/j.1365-2966.2008.14023.x
Abstract
We discuss an approach to the component separation of microwave, multi-frequency sky maps as those typically produced from Cosmic Microwave Background (CMB) Anisotropy data sets. The algorithm is based on the two step, parametric, likelihood-based technique recently elaborated on by Eriksen et al., (2006), where the foreground spectral parameters are estimated prior to the actual separation of the components. In contrast with the previous approaches, we accomplish the former task with help of an analytically-derived likelihood function for the spectral parameters, which, we show, yields estimates equal to the maximum likelihood values of the full multi-dimensional data problem. We then use these estimates to perform the second step via the standard, generalized-least-square-like procedure. We demonstrate that the proposed approach is equivalent to a direct maximization of the full data likelihood, which is recast in a computationally tractable form. We use the corresponding curvature matrices to characterize statistical properties of the recovered parameters. We incorporate in the formalism some of the essential features of the CMB data sets, such as inhomogeneous pixel domain noise, unknown map offsets as well as calibration errors and study their consequences for the separation. We find that the calibration is likely to have a dominant effect on the precision of the spectral parameter determination for a realistic CMB experiment. We apply the algorithm to simulated data and discuss the results. Our focus is on partial-sky, total-intensity and polarization, CMB experiments such as planned balloon-borne and ground-based efforts, however, the techniques presented here should be also applicable to the full-sky data as for instance, those produced by WMAP and anticipated from Planck.
18 pages, 8 figures, minor changes to match the published version
References in corpus (29)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Efficient Computation of CMB anisotropies in closed FRW models
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- An All-Sky Analysis of Polarization in the Microwave Background
- Weak Gravitational Lensing of the CMB
- Statistics of Cosmic Microwave Background Polarization
- Extrapolation of Galactic Dust Emission at 100 Microns to CMBR Frequencies Using FIRAS
- Gravitational Lensing Effect on Cosmic Microwave Background Polarization
- Estimating the Power Spectrum of the Cosmic Microwave Background
- Joint Bayesian component separation and CMB power spectrum estimation
- Multi-Detector Multi-Component spectral matching and applications for CMB data analysis
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization
- CMB component separation by parameter estimation
- First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops
- MAXIPOL: Cosmic Microwave Background Polarimetry Using a Rotating Half-Wave Plate
- The EBEX Experiment
- New Measurements of Fine-Scale CMB Polarization Power Spectra from CAPMAP at Both 40 and 90 GHz
- Making Maps Of The Cosmic Microwave Background: The MAXIMA Example
- First season QUaD CMB temperature and polarization power spectra
- Making sky maps from Planck data
- Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops
- Foreground Subtraction of Cosmic Microwave Background Maps using WI-FIT (Wavelet based hIgh resolution Fitting of Internal Templates)
- All-sky component separation in the presence of anisotropic noise and dust temperature variations
- Estimating the spectral indices of correlated astrophysical foregrounds by a second-order statistical approach
- CMB signal in WMAP 3yr data with FastICA
- Determining Foreground Contamination in CMB Observations: Diffuse Galactic Emission in the MAXIMA-I Field
Cited by in corpus (76)
- Planck 2013 results. XII. Component separation
- The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
- Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
- CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
- Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers
- EBEX: A balloon-borne CMB polarization experiment
- MADmap: A Massively Parallel Maximum-Likelihood Cosmic Microwave Background Map-Maker
- Exploring Cosmic Origins with CORE: B-mode Component Separation
- The C-Band All-Sky Survey (C-BASS): Design and capabilities
- Cosmic bulk flows on 50 {h}^{-1}Mpc scales: A Bayesian hyper-parameter method and multishells likelihood analysis
- Forecasting performance of CMB experiments in the presence of complex foreground contaminations
- Evidence for extra radiation? Profile likelihood versus Bayesian posterior
- A minimal power-spectrum-based moment expansion for CMB B-mode searches
- Modeling atmospheric emission for CMB ground-based observations
- Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
- Maximum likelihood, parametric component separation and CMB B-mode detection in suborbital experiments
- Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
- Simulated forecasts for primordial B-mode searches in ground-based experiments
- The Simons Observatory: Galactic Science Goals and Forecasts
- The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
- The Simons Observatory: pipeline comparison and validation for large-scale B-modes
- BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
- A Model For Polarised Microwave Foreground Emission From Interstellar Dust
- Framework for performance forecasting and optimization of CMB B-mode observations in presence of astrophysical foregrounds
- LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
- BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors
- Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
- Multi-Clustering Needlet-ILC for CMB B-modes component separation
- Framework for analysis of next generation, polarised CMB data sets in the presence of galactic foregrounds and systematic effects
- Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
- Principal component analysis of the primordial tensor power spectrum
- LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
- Optimization Study for the Experimental Configuration of CMB-S4
- Astrophysical foregrounds and primordial tensor-to-scalar ratio constraints from CMB B-mode polarization observations
- Foreground model recognition through Neural Networks for CMB B-mode observations
- The Effects of Bandpass Variations on Foreground Removal Forecasts for Future CMB Experiments
- Characterising cosmic birefringence in the presence of galactic foregrounds and instrumental systematic effects
- Forecast B-modes detection at large scales in presence of noise and foregrounds
- Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods
- Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data
- Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
- Estimating the tensor-to-scalar ratio and the effect of residual foreground contamination
- Requirements for future CMB satellite missions: photometric and band-pass response calibration
- A hybrid map- component separation method for primordial CMB -mode searches
- Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
- Analysis of NILC performance on B-modes data of sub-orbital experiments
- Testing for spectral index variations in polarised CMB foregrounds
- Impact of modelling foreground uncertainties on future CMB polarization satellite experiments
- Recent developments in astrophysical and cosmological exploitation of microwave surveys
- Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
- How bad could it be? Modelling the 3D complexity of the polarised dust signal using moment expansion
- Foreground removal with ILC methods for AliCPT-1
- Non-parametric maximum likelihood component separation for CMB polarization data
- Forecast of foreground cleaning strategies for AliCPT-1
- The Superhorizon Test of Future B-mode Experiments
- Detecting the tensor-to-scalar ratio with the pure pseudospectrum reconstruction of -mode
- Foreground removal requirements for measuring large-scale CMB B-modes in light of BICEP2
- The information content of Cosmic Infrared Background anisotropies
- A Constrained NILC method for CMB B mode observations
- Identifying frequency decorrelated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry
- Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
- Accelerating linear system solvers for time domain component separation of cosmic microwave background data
- Extended Delta-map: a map-based foreground removal method for CMB polarization observations
- ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
- Deep Needlet: A CNN based full sky component separation method in Needlet space
- Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments
- Dark matter search with CMB: a study of foregrounds
- The Bayesian Global Sky Model (B-GSM): Validation of a Data Driven Bayesian Simultaneous Component Separation and Calibration Algorithm for EoR Foreground Modelling
- Requirements on bandpass resolution and measurement precision for LiteBIRD
- Estimating the Impact of foregrounds on the Future Detection of Rayleigh scattering
- Bayesian recalibration of flux scale factors in diffuse radio maps using low-resolution absolute radiometers
- Cosmic Microwave Background Science at Commercial Airline Altitudes
- LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
- Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
- Accurate and efficient likelihood modeling for large-scale CMB data
- The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science