English

Frabjous: Deep Learning Fast Radio Burst Morphologies

Instrumentation and Methods for Astrophysics 2026-04-08 v2 High Energy Astrophysical Phenomena

Abstract

The increasing field of view of radio telescopes and improved data processing capabilities have led to a surge in the detection of Fast Radio Bursts (FRBs). The discovery rate of FRBs is already a few per day and is expected to increase rapidly with new surveys coming online. The growing number of events necessitates prioritized follow-up due to limited multi-wavelength resources, requiring rapid and automated classification. In this study, we introduce Frabjous, a deep learning framework for an automated morphology classifier with an aim towards enabling the prompt follow-up of anomalous and intriguing FRBs, and a comprehensive statistical analysis of FRB morphologies. Deep learning models require a large training set of each FRB archetype, however, publicly available data lacks sufficient samples for most FRB types. In this paper, we build a simulation framework for generating realistic examples of FRBs and train a network based on a combination of simulated and real data, starting with the CHIME/FRB catalog. Applying our framework to the first CHIME/FRB catalog, we achieve an overall classification accuracy of approximately 55%, well over a random multiclass classification rate of 20 % with five balanced classes during training. While this falls short of desirable performance, we critically discuss the limitations of our approach and propose potential avenues for improvement. Future work should explore strategies to augment training datasets and broaden the scope of FRB morphological studies, aiming for more accurate and reliable classification results.

Keywords

Cite

@article{arxiv.2507.14854,
  title  = {Frabjous: Deep Learning Fast Radio Burst Morphologies},
  author = {Ajay Kumar and Ashish A. Mahabal and Shriharsh P. Tendulkar},
  journal= {arXiv preprint arXiv:2507.14854},
  year   = {2026}
}

Comments

22 pages, 17 figues, 3 tables, Accepted for publication in PASA

R2 v1 2026-07-01T04:09:45.340Z