Sparsity and adaptivity for the blind separation of partially correlated sources
arXiv:1412.4005 · doi:10.1109/TSP.2015.2391071
Abstract
Blind source separation (BSS) is a very popular technique to analyze multichannel data. In this context, the data are modeled as the linear combination of sources to be retrieved. For that purpose, standard BSS methods all rely on some discrimination principle, whether it is statistical independence or morphological diversity, to distinguish between the sources. However, dealing with real-world data reveals that such assumptions are rarely valid in practice: the signals of interest are more likely partially correlated, which generally hampers the performances of standard BSS methods. In this article, we introduce a novel sparsity-enforcing BSS method coined Adaptive Morphological Component Analysis (AMCA), which is designed to retrieve sparse and partially correlated sources. More precisely, it makes profit of an adaptive re-weighting scheme to favor/penalize samples based on their level of correlation. Extensive numerical experiments have been carried out which show that the proposed method is robust to the partial correlation of sources while standard BSS techniques fail. The AMCA algorithm is evaluated in the field of astrophysics for the separation of physical components from microwave data.
arXiv commentsubmitted to IEEE Transactions on signal processing
References in corpus (11)
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
- Wavelets, ridgelets and curvelets on the sphere
- Foregrounds and CMB Experiments: I. Semi-analytical estimates of contamination
- Sparse and Unique Nonnegative Matrix Factorization Through Data Preprocessing
- SZ and CMB reconstruction using Generalized Morphological Component Analysis
- Joint Planck and WMAP CMB Map Reconstruction
- Sparse component separation for accurate CMB map estimation
- Exact and Heuristic Algorithms for Semi-Nonnegative Matrix Factorization
- Sparse and Non-Negative BSS for Noisy Data
- WMAP 9-year CMB estimation using sparsity
Cited by in corpus (21)
- Recovery of 21 cm intensity maps with sparse component separation
- Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
- CMB reconstruction from the WMAP and Planck PR2 data
- A novel method for component separation of extended sources in X-ray astronomy
- ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
- Robust Sparse Blind Source Separation
- The SRG/eROSITA diffuse soft X-ray background. I. The local hot bubble in the western Galactic hemisphere
- Three-dimensional morphological asymmetries in the ejecta of Cassiopeia A using a component separation method in X-rays
- Joint Multichannel Deconvolution and Blind Source Separation
- Asymmetries of Heavy Elements in the Young Supernova Remnant Cassiopeia A
- H-X-ray Surface Brightness Correlation for Filaments in Cooling Flow Clusters
- A fresh perspective on the 3D dynamics of Tycho's supernova remnant: Ejecta asymmetries in the X-ray band
- The X-ray synchrotron rims in Cassiopeia A narrow with energy
- Joint deconvolution and unsupervised source separation for data on the sphere
- Provably robust blind source separation of linear-quadratic near-separable mixtures
- Comparing the three-dimensional morphological asymmetries in the ejecta of Kepler and Tycho in X-rays
- Heuristics for Efficient Sparse Blind Source Separation
- Exploring Bounded Component Analysis Using an Norm Criterion
- Direct observation of the X-ray counterpart of the Hα filaments and of the sloshing spiral in the Perseus galaxy cluster
- Measurements of the diffuse Galactic synchrotron spectral index and curvature from MeerKLASS pilot data
- Joint deconvolution and blind source separation on the sphere with an application to radio-astronomy