| Issue |
A&A
Volume 705, January 2026
|
|
|---|---|---|
| Article Number | A226 | |
| Number of page(s) | 11 | |
| Section | Numerical methods and codes | |
| DOI | https://doi.org/10.1051/0004-6361/202556228 | |
| Published online | 23 January 2026 | |
LCS: A learnlet-based sparse framework for blind source separation
1
Institutes of Computer Science and Astrophysics, Foundation for Research and Technology Hellas (FORTH),
Greece
2
Université Paris-Saclay, Université Paris Cité, CEA, CNRS,
AIM,
91191
Gif-sur-Yvette,
France
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
3
July
2025
Accepted:
22
November
2025
Blind source separation (BSS) plays a pivotal role in modern astrophysics by enabling the extraction of scientifically meaningful signals from multi-frequency observations. Traditional BSS methods, such as those that rely on fixed wavelet dictionaries, enforce sparsity during component separation but can fall short when faced with the inherent complexity of real astrophysical signals. In this work, we introduce the learnlet component separator (LCS), a novel BSS framework that bridges classical sparsity-based techniques and modern deep learning. LCS utilises the learnlet transform – a structured convolutional neural network designed to serve as a learned, wavelet-like multi-scale representation. This hybrid design preserves the interpretability and sparsity-promoting properties of wavelets while gaining the adaptability and expressiveness of learned models. The LCS algorithm integrates this learned sparse representation into an iterative source separation process, enabling the effective decomposition of multi-channel observations. While conceptually inspired by sparse BSS methods, LCS introduces a learned representation layer that significantly departs from classical fixed-basis assumptions. We evaluated LCS on both synthetic and real datasets and in this paper demonstrate its superior separation performance compared to state-of-the-art methods (average gain of about 5 dB on toy model examples). Our results highlight the potential of hybrid approaches that combine signal processing priors with deep learning to address the challenges of next-generation cosmological experiments.
Key words: methods: data analysis / methods: statistical / techniques: image processing
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. This email address is being protected from spambots. You need JavaScript enabled to view it. to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.