DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: A novel CMB component separation method: hierarchical generalized morphological component analysis

Journal Article · · Monthly Notices of the Royal Astronomical Society
ORCiD logo [1];  [2];  [3];  [3]
  1. Department of Physics, Harvard University, Cambridge, MA 02138, USA, Department of Physics, Stanford University, Stanford, CA 94305, USA
  2. Department of Mathematics, Harvard University, Cambridge, MA 02138, USA, Department of Computer Science and Engineering, University of California San Diego, San Diego, CA 92092, USA
  3. Department of Physics, Harvard University, Cambridge, MA 02138, USA

ABSTRACT We present a novel technique for cosmic microwave background (CMB) foreground subtraction based on the framework of blind source separation. Inspired by previous work incorporating local variation to generalized morphological component analysis (GMCA), we introduce hierarchical GMCA (HGMCA), a Bayesian hierarchical graphical model for source separation. We test our method on Nside = 256 simulated sky maps that include dust, synchrotron, free–free, and anomalous microwave emission, and show that HGMCA reduces foreground contamination by $$25{{\ \rm per\ cent}}$$ over GMCA in both the regions included and excluded by the Planck UT78 mask, decreases the error in the measurement of the CMB temperature power spectrum to the 0.02–0.03 per cent level at ℓ > 200 (and $$\lt 0.26{{\ \rm per\ cent}}$$ for all ℓ), and reduces correlation to all the foregrounds. We find equivalent or improved performance when compared to state-of-the-art internal linear combination type algorithms on these simulations, suggesting that HGMCA may be a competitive alternative to foreground separation techniques previously applied to observed CMB data. Additionally, we show that our performance does not suffer when we perturb model parameters or alter the CMB realization, which suggests that our algorithm generalizes well beyond our simplified simulations. Our results open a new avenue for constructing CMB maps through Bayesian hierarchical analysis.

Sponsoring Organization:
USDOE; National Science Foundation (NSF)
Grant/Contract Number:
SC0020223
OSTI ID:
1632766
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 494; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United Kingdom
Language:
English

References (48)

Wavelets on the 2-Sphere: A Group-Theoretical Approach journal November 1999
Diffuse Source Separation in CMB Observations book January 2008
Independent component analysis: algorithms and applications journal June 2000
Localisation of directional scale-discretised wavelets on the sphere journal January 2018
Cosmic microwave background power spectrum estimation and map reconstruction with the expectation-maximization algorithm journal November 2003
Foreground separation methods for satellite observations of the cosmic microwave background journal October 1998
Sparse component separation for accurate cosmic microwave background estimation journal January 2013
S2LET: A code to perform fast wavelet analysis on the sphere journal October 2013
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect journal October 2014
Planck 2013 results. I. Overview of products and scientific results journal October 2014
Planck 2013 results. XII. Diffuse component separation journal October 2014
Planck 2013 results. XVI. Cosmological parameters journal October 2014
Joint Planck and WMAP CMB map reconstruction journal March 2014
Planck 2015 results : XIII. Cosmological parameters journal September 2016
Planck 2015 results : X. Diffuse component separation: Foreground maps journal September 2016
Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters journal September 2016
Planck 2015 results : XII. Full focal plane simulations journal September 2016
Component separation methods for the PLANCK mission journal October 2008
A full sky, low foreground, high resolution CMB map from WMAP journal November 2008
Power Spectrum of Primordial Inhomogeneity Determined from the FOUR-Year [ITAL]COBE[/ITAL] DMR Sky Maps journal June 1996
Power Spectrum Estimation from High‐Resolution Maps by Gibbs Sampling journal December 2004
HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the Sphere journal April 2005
Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data journal June 2006
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: BAYESIAN ESTIMATION OF COSMIC MICROWAVE BACKGROUND POLARIZATION MAPS journal August 2009
SPATIAL VARIATIONS IN THE SPECTRAL INDEX OF POLARIZED SYNCHROTRON EMISSION IN THE 9 yr WMAP SKY MAPS journal July 2014
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS journal September 2013
A Multi-Level Solver for Gaussian Constrained Cosmic Microwave Background Realizations journal January 2014
A needlet ILC analysis of WMAP 9-year polarization data: CMB polarization power spectra journal August 2013
SILC: a new Planck internal linear combination CMB temperature map using directional wavelets journal May 2016
Spin-SILC: CMB polarization component separation with spin wavelets journal August 2016
Wavelet-Bayesian inference of cosmic strings embedded in the cosmic microwave background journal September 2017
The Python Sky Model: software for simulating the Galactic microwave sky journal May 2017
High resolution foreground cleaned CMB map from WMAP journal December 2003
How Isotropic is the Universe? journal September 2016
A Novel Sampling Theorem on the Rotation Group journal December 2015
A Novel Sampling Theorem on the Sphere journal December 2011
Sparse and Non-Negative BSS for Noisy Data journal November 2013
Second-Generation Curvelets on the Sphere journal January 2017
Multidetector multicomponent spectral matching and applications for cosmic microwave background data analysis journal December 2003
Template fitting and the large-angle cosmic microwave background anomalies journal April 2006
Exact reconstruction with directional wavelets on the sphere journal August 2008
A needlet internal linear combination analysis of WMAP 7-year data: estimation of CMB temperature map and power spectrum: A NILC analysis of WMAP 7-year data journal November 2011
Localized Tight Frames on Spheres journal January 2006
Linear Inversion of Band-Limited Reflection Seismograms journal October 1986
Separation of Correlated Astrophysical Sources Using Multiple-Lag Data Covariance Matrices journal September 2005
Blind Component Separation in Wavelet Space: Application to CMB Analysis journal September 2005
Bayesian Data Analysis book November 2013
Asymptotics for spherical needlets journal June 2009

Similar Records

Multiclustering needlet ILC for CMB B -mode component separation
Journal Article · 2023 · Monthly Notices of the Royal Astronomical Society · OSTI ID:1998200

Quantifying bias due to non-Gaussian foregrounds in an optimal reconstruction of CMB lensing and temperature power spectra
Journal Article · 2025 · Journal of Cosmology and Astroparticle Physics · OSTI ID:2998879

Extracting cosmic microwave background polarization from satelliteastrophysical maps
Journal Article · 2004 · Monthly Notices of the Royal Astronomical Society · OSTI ID:893509

Related Subjects