Convolutional Deep Denoising Autoencoders for Radio Astronomical Images
Claudio Gheller, Franco Vazza

TL;DR
This paper demonstrates that convolutional denoising autoencoders can effectively reduce noise and artefacts in radio astronomical images, enabling detection of faint, extended sources in large datasets with high accuracy.
Contribution
The study introduces a convolutional denoising autoencoder tailored for radio astronomy, capable of handling complex noise and artefacts, and scalable for large observational datasets.
Findings
Effectively denoises complex radio images
Accurately detects faint, extended sources
Scales efficiently on large datasets
Abstract
We apply a Machine Learning technique known as Convolutional Denoising Autoencoder to denoise synthetic images of state-of-the-art radio telescopes, with the goal of detecting the faint, diffused radio sources predicted to characterise the radio cosmic web. In our application, denoising is intended to address both the reduction of random instrumental noise and the minimisation of additional spurious artefacts like the sidelobes, resulting from the aperture synthesis technique. The effectiveness and the accuracy of the method are analysed for different kinds of corrupted input images, together with its computational performance. Specific attention has been devoted to create realistic mock observations for the training, exploiting the outcomes of cosmological numerical simulations, to generate images corresponding to LOFAR HBA 8 hours observations at 150 MHz. Our autoencoder can…
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Taxonomy
MethodsDenoising Autoencoder
