English

Gamma-ray burst light curve reconstruction with predictive models

High Energy Astrophysical Phenomena 2026-01-30 v1 Instrumentation and Methods for Astrophysics

Abstract

Gamma-ray bursts represent some of the most energetic and complex phenomena in the universe, characterized by highly variable light curves that often contain observational gaps. Reconstructing these light curves is essential for gaining deeper insight into the physical processes driving such events. This study proposes a machine learning-based framework for the reconstruction of gamma-ray burst light curves, focusing specifically on the plateau phase observed in X-ray data. The analysis compares the performance of three sequential modeling approaches: a bidirectional recurrent neural network, a gated recurrent architecture, and a convolutional model designed for temporal data. The findings of this study indicate that the Bidirectional Gated Recurrent Unit model showed the best predictive accuracy among the evaluated models across all GRB types, as measured by Mean Absolute Error, Root Mean Square Error, and Coefficient of Determination. Notably, Bidirectional Gated Recurrent Unit exhibited enhanced capability in modeling both gradual plateau phases and abrupt transient features, including flares and breaks, particularly in complex light-curve scenarios.

Keywords

Cite

@article{arxiv.2508.16924,
  title  = {Gamma-ray burst light curve reconstruction with predictive models},
  author = {Zhunuskanov A. and Sakan A. and Akhmetali A. and Zaidyn M. and Ussipov N},
  journal= {arXiv preprint arXiv:2508.16924},
  year   = {2026}
}

Comments

13 pages, 7 figures, 2 tables

R2 v1 2026-07-01T05:02:42.157Z