Journal Article2026

RGC: A radio AGN classifier based on deep learning

M. S. Hossain, M. S. H. Shahal, K. M. B. Asad, P. Saikia, A. Khan, F. Akter, A. A. Ali, M. A. Amin, D. P. Guha, M. Hasan, M. O. B. Jihad, A. Momen, S. Sen, A. K. M. M. Rahman

Astronomy & Astrophysics

EDP Sciences, Vol. 714, pp. A5, ISBN: 0004-6361

Abstract

Context . Bent radio active galactic nuclei (RAGNs) – wide-angle tails (WATs) and narrow-angle tails (NATs) – trace dense environments in galaxy groups and clusters, yet no multi-class classifier simultaneously separates them from straight Fanaroff-Riley types (sFRI, sFRII) using visually inspected labels and unlabelled data. Aims . We release FIRST-2060, a four-class labelled dataset of 2060 RAGNs (sFRI, sFRII, WAT, NAT) constructed from three publicly available catalogues through multi-tier visual inspection, together with the semi-supervised RGC 1.0 model that leverages 20 000 unlabelled radio sources. We benchmarked RGC 1.0 against five supervised baselines spanning convolutional neural networks (CNNs) and vision transformers. Methods . FIRST-2060 is provided in two preprocessing variants: R L 1 , which retains spurious sources, and R L 2 , from which they are removed. The RGC model integrates the self-supervised framework Bootstrap Your Own Latent (BYOL) with an E (2)-equivariant steerable CNN (E2CNN) encoder, pre-trained on the unlabelled data and fine-tuned on the labelled sets. All six models were evaluated with five-fold cross-validation, gradient-weighted class activation mapping (Grad-CAM) attention analysis, and controlled class-imbalance experiments. Results . ConvNeXT ( M 1 ) and RGC ( M 2 ) form a top tier at macro- F 1 0.80 ± 0.02 and 0.79 ± 0.02, respectively, representing a difference within one standard deviation. The RGC model is the only model whose Grad-CAM contours consistently trace the morphological structure of RAGNs – lobes, jets, and bends – rather than defaulting to compact blobs or diffuse patterns. Conclusions . The four-class scheme introduced here enables WAT and NAT resolved catalogues that can serve as environment probes and progenitor classifications for diffuse cluster radio emission. The complementary strengths of M 1 and M 2 – in cross-type and within-type discrimination, respectively – suggest that an ensemble approach may offer a practical framework for survey-scale morphological catalogues.

Keywords

  • radio galaxy morphology
  • semi-supervised classification
  • multi-class classifier
  • radio galaxy environment

CCDS Authors

Prof. M Ashraful Amin, PhD
M Ashraful Amin, PhD

Prof. M Ashraful Amin, PhD

  • Founder Director, CCDS
  • Director, AI/ML, HCI & DS Wings

Published at

ACL, CHI, UbiComp, ECAI, WACV, PAKDD, IJCNN, ICPR, ICIP, HCII, CLEF, BLP, Scientific Reports, Pattern Recognition, JMIR, IEEE Access, Smart Agricultural Technology, Frontiers in Computational Neuroscience, Diabetes Research and Clinical Practice, PLOS ONE

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