Aug 2026· Monthly Notices of the Royal Astronomical Society· Vol 551· 0 citations· 18 references
Physics
TL;DR
This work presents YOLO-Chars (YOLO-based Detection and Characterisation of Radio Sources), a two-stage deep-learning framework for the automated detection and characterisation of radio galaxies in survey images using the Square Kilometre Array Science Data Challenge 1 dataset.
Abstract
Future radio telescopes will generate data volumes that are increasingly difficult to analyse using traditional statistical methods, motivating the adoption of machine-learning techniques. In this work, we present YOLO-Chars (YOLO-based Detection and Characterisation of Radio Sources), a two-stage deep-learning framework for the automated detection and characterisation of radio galaxies in survey images. The framework is developed and evaluated using the Square Kilometre Array Science Data Challenge 1 (SKA SDC1) dataset. In the first stage, customised YOLO-based multi-scale detection models are used to localise compact and extended sources across large sky maps. In the second stage, a dedicated source-characterisation network estimates the physical properties of the detected sources. We focus on three key parameters: flux density, angular size, and position angle. Our results show that YOLO-Chars achieves competitive detection and characterisation performance on the SKA SDC1 benchmark, demonstrating its potential as a scalable framework for next-generation radio continuum surveys.
We present FM-JADES-v1, a self-supervised foundation model for James Webb Space Telescope ({\em JWST}) deep-field science, trained with 482,444 objects from the {\em JWST} Advanced Deep Extragalactic Survey (JADES) Data Release 5 using multi-band imaging and the photometric catalog. The shared embedding space is traine...
Jia-Ni Ding, M. Yue, Yong-Da Zhu et al.· 1 citation
Galaxy clusters are the most powerful strong lenses; they greatly magnify the flux of distant and faint sources. Strong lensing also allows for the reconstruction of their mass distribution with sim1% accuracy and enables the investigation of cosmological parameters. The number of known systems of this type is bound to...
L. Leuzzi, M. Meneghetti, A. Adam et al.· Astronomy & Astrophysics· 0 citations
The Cherenkov Telescope Array Observatory (CTAO) marks the next generation of Imaging Atmospheric Cherenkov Telescopes (IACTs), offering a sensitivity improvement of up to a factor of 10 over current instruments. Its first prototype, the Large-Sized Telescope (LST-1), is already in operation at the Roque de los Muchach...
G. Grolleron, C. Plard, M. Dell'aiera et al.· 0 citations
In this work, we present a novel deep learning-based approach for the detection of changing-state quasars (CSQSOs), which are of critical importance in quasars (QSOs) research due to their substantial temporal variations in optical properties. Detecting and monitoring CSQSOs presents considerable challenges, including...
A variational auto-encoder (VAE) with a normalising flow is constructed, developing a specific training loss function for the VAE in both the direct and Fourier spaces, which has enabled the construction of the small-scale and thin features associated with the gravitational interaction between merging galaxies like tid...
C. Mahé, H. Bretonnière, E. Slezak· Astronomy & Astrophysics· 0 citations
The embedded position of each galaxy can be identified $>100$ times faster than inferring its properties with Bayesian SED fitting, making this approach an ideal alternative for deriving statistical model constraints from large surveys such as LSST and Euclid, and performing simulation-based inference with CAMELS.
Jack C. Turner, S. Wilkins, W. Roper et al.· 0 citations
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