English

Denoising radio pulses from air showers using machine-learning methods

Instrumentation and Methods for Astrophysics 2025-07-10 v1 High Energy Astrophysical Phenomena

Abstract

The Giant Radio Array for Neutrino Detection (GRAND) aims to detect radio signals from extensive air showers (EAS) caused by ultra-high-energy (UHE) cosmic particles. Galactic, hardware-like, and anthropogenic noise are expected to contaminate these signals. To address this problem, we propose training a supervised convolutional network known as an encoder-decoder. This network is used to learn a coded representation of the data and remove specific features from it. This denoiser is trained using high-fidelity air shower simulations specifically tailored to replicate the characteristics of signals detected by GRAND. In this contribution, we describe our machine-learning model and report initial results demonstrating the sensitivity enhancement resulting from our denoising algorithm when applied to realistically simulated GRAND signals with varying signal-to-noise ratios.

Keywords

Cite

@article{arxiv.2507.06688,
  title  = {Denoising radio pulses from air showers using machine-learning methods},
  author = {Aurélien Benoit-Lévy and Zhisen Lai and Oscar Macias and Arsène Ferrière},
  journal= {arXiv preprint arXiv:2507.06688},
  year   = {2025}
}

Comments

Presented at the 39th International Cosmic Ray Conference (ICRC 2023). 10 pages, 6 figures

R2 v1 2026-07-01T03:52:54.844Z