Cosmological constraints from noisy convergence maps through deep learning
Janis Fluri, Tomasz Kacprzak, Aurelien Lucchi, Alexandre Refregier,, Adam Amara, Thomas Hofmann (ETH Zurich)

TL;DR
This paper demonstrates that convolutional neural networks can extract more precise cosmological parameters from noisy weak lensing maps than traditional power spectrum methods, especially at lower noise levels and smaller smoothing scales.
Contribution
It introduces a new deep learning approach with a specialized training strategy that outperforms power spectrum analysis in constraining cosmological parameters from noisy convergence maps.
Findings
CNN achieves up to 50% tighter constraints than power spectrum.
Performance advantage decreases with higher noise and larger smoothing scales.
Proposes a new training method for neural networks with noisy data.
Abstract
Deep learning is a powerful analysis technique that has recently been proposed as a method to constrain cosmological parameters from weak lensing mass maps. Due to its ability to learn relevant features from the data, it is able to extract more information from the mass maps than the commonly used power spectrum, and thus achieve better precision for cosmological parameter measurement. We explore the advantage of Convolutional Neural Networks (CNN) over the power spectrum for varying levels of shape noise and different smoothing scales applied to the maps. We compare the cosmological constraints from the two methods in the plane for sets of 400 deg convergence maps. We find that, for a shape noise level corresponding to 8.53 galaxies/arcmin and the smoothing scale of arcmin, the network is able to generate 45% tighter constraints. For…
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