Abstract

We present a new machine learning (ML)-driven source-finding tool for next-generation radio surveys that performs fast source extraction on a range of source morphologies at large dynamic ranges with minimal parameter tuning and post-processing. The construction of the Square Kilometre Array (SKA) radio telescope will revolutionize the field of radio astronomy. However, accurate and automated source-finding techniques are required to reach SKA science goals. We have developed a novel source-finding method, ContinUNet, powered by an ML segmentation algorithm, U-Net, that has proven highly effective and efficient when tested on SKA precursor data sets. Our model was trained and tested on simulated radio continuum data from SKA Science Data Challenge 1 and proved comparable with the state-of-the-art source-finding methods, PyBDSF and ProFound. ContinUNet was then tested on the MeerKAT International GHz Tiered Extragalactic Exploration Early Science data without retraining and was able to extract point-like and extended sources with equal ease; processing a 1.6 deg$^2$ field in $\lt $13 s on a supercomputer and $\approx$2 min on a personal laptop. We were able to associate components of extended sources without manual intervention with the powerful inference capabilities learnt within the network, making ContinUNet a promising tool for enabling science in the upcoming SKA era.

Details

Title
ContinUNet: fast deep radio image segmentation in the Square Kilometre Array era with U-Net
Author
Stewart, Hattie 1   VIAFID ORCID Logo  ; Birkinshaw, Mark 1 ; Siu-Lun Yeung 2 ; Maddox, Natasha 1 ; Maughan, Ben 1   VIAFID ORCID Logo  ; Thiyagalingam, Jeyan 2 

 School of Physics, University of Bristol , HH Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL , UK 
 SciML, Scientific Computing Department, Research Complex at Harwell, Rutherford Appleton Laboratory , Harwell Oxford, Didcot OX11 0FA , UK 
Pages
315-332
Publication year
2024
Publication date
Jan 2024
Publisher
Oxford University Press
e-ISSN
27528200
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3191364159
Copyright
© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.