TL;DR
This paper introduces a novel multi-scale decomposition method for astronomical maps using a constrained diffusion approach, addressing artifacts in wave transforms and enabling better analysis of localized, non-linear features.
Contribution
The authors develop a non-linear diffusion-based decomposition method that guarantees positivity and is tailored for astronomical signals, with an accompanying scale spectrum measure.
Findings
Addresses artifact issues in wave transform decompositions.
Guarantees positivity of decomposed components.
Provides a practical Python implementation.
Abstract
We propose a new, efficient multi-scale method to decompose a map (or signal in general) into components maps that contain structures of different sizes. In the widely-used wave transform, artifacts containing negative values arise around regions with sharp transitions due to the application of band-limited filters. In our approach, the decomposition is achieved by solving a modified, non-linear version of the diffusion equation. This is inspired by the anisotropic diffusion methods, which establish the link between image filtering and partial differential equations. In our case, the artifact issue is addressed where the positivity of the decomposed images is guaranteed. Our new method is particularly suitable for signals which contain localized, non-linear features, as typical of astronomical observations. It can be used to study the multi-scale structures of astronomical maps…
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