Convolutional Deep Denoising Autoencoders for Radio Astronomical Images
- URL: http://arxiv.org/abs/2110.08618v1
- Date: Sat, 16 Oct 2021 17:08:30 GMT
- Title: Convolutional Deep Denoising Autoencoders for Radio Astronomical Images
- Authors: Claudio Gheller and Franco Vazza
- Abstract summary: We apply a Machine Learning technique known as Convolutional Denoising Autoencoder to denoise synthetic images of state-of-the-art radio telescopes.
Our autoencoder can effectively denoise complex images identifying and extracting faint objects at the limits of the instrumental sensitivity.
- Score: 0.0
- License: http://creativecommons.org/licenses/by/4.0/
- 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 effectively denoise
complex images identifying and extracting faint objects at the limits of the
instrumental sensitivity. The method can efficiently scale on large datasets,
exploiting high performance computing solutions, in a fully automated way (i.e.
no human supervision is required after training). It can accurately perform
image segmentation, identifying low brightness outskirts of diffused sources,
proving to be a viable solution for detecting challenging extended objects
hidden in noisy radio observations.
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