| Issue |
A&A
Volume 701, September 2025
|
|
|---|---|---|
| Article Number | A170 | |
| Number of page(s) | 14 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/202554142 | |
| Published online | 12 September 2025 | |
Generative modelling of convergence maps based on predicted one-point statistics
1
Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191 Gif-sur-Yvette, France
2
Institutes of Computer Science and Astrophysics, Foundation for Research and Technology Hellas (FORTH), Heraklion, Crete, Greece
⋆ Corresponding author: vilasini.tinnanerisreekanth@cea.fr
Received:
14
February
2025
Accepted:
6
July
2025
Context. Weak gravitational lensing is a key cosmological probe for current and future large-scale surveys. While power spectra are commonly used for analyses, they fail to capture non-Gaussian information from non-linear structure formation, which necessitates higher-order statistics and methods for an efficient map generation.
Aims. We develop an emulator that generates accurate convergence (κ) maps directly from an input power spectrum and wavelet ℓ1-norm without relying on computationally intensive simulations.
Methods. We used either numerical or theoretical predictions to construct κ maps by iteratively adjusting the wavelet coefficients to match the marginal distributions of the target and their inter-scale dependences by incorporating higher-order statistical information.
Results. The resulting κ maps accurately reproduce the input power spectrum, and their higher-order statistical properties are consistent with the input predictions. They thus provide an efficient tool for weak-lensing analyses.
Key words: cosmology: theory / large-scale structure of Universe
© The Authors 2025
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.
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