activity
20092026
most citedTowards online triggering for the radio detection of air showers using deep neural networks

5 citations · 12 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2026

Energy estimation of direct and reflected cosmic-ray events aboard balloon-borne radio detectors

Sergio Cabana-Freire, Jaime Alvarez-Muñiz, Matias Tueros

Balloon-borne radio detectors offer a highly effective approach to monitoring immense volumes of the Earth's atmosphere and ice for ultra-high-energy cosmic rays and neutrinos. Bec…

astro-ph.IM2026

Reconstruction of cosmic-ray direction and energy in radio arrays using deep ensemble graph neural networks

Arsène Ferrière, Aurélien Benoit-Lévy, Olivier Martineau-Huynh +1

Using advanced machine learning techniques, we developed a method to reconstruct the arrival direction and energy of ultra-high-energy cosmic rays from the voltage traces they indu…

hep-ex2026

Deep-Learning Denoising of Radio Signals for Ultra-High-Energy Cosmic-Ray Detection

Zhisen Lai, Oscar Macias, Aurélien Benoit-Lévy +2

Extensive air showers initiated by ultra-high-energy cosmic rays (UHECRs) produce broadband radio pulses detectable over large areas, but Galactic and instrumental backgrounds limi…

astro-ph.HE2026

Radio Morphing: Fast computation of inclined air shower radio emission

Simon Chiche, Olivier Martineau-Huynh, Matias Tueros +1

The preparation of the next-generation of large-scale radio experiments requires running a large number of simulations to explore multiple detector configurations over vast areas a…

astro-ph.IM2025★ 2 cited

Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes

GRAND Collaboration, Jaime Álvarez-Muniz, Rafael Alves Batista +118

The Giant Radio Array for Neutrino Detection (GRAND) is a proposed multi-messenger observatory of Ultra-High-Energy (UHE) particles of cosmic origin. Its main goal is to find the l…

astro-ph.HE2025

Simulation-Based Inference for Direction Reconstruction of Ultra-High-Energy Cosmic Rays with Radio Arrays

Oscar Macias, Zachary Mason, Matthew Ho +3

Ultra-high-energy cosmic-ray (UHECR) observatories require unbiased direction reconstruction to enable multi-messenger astronomy with sparse, nanosecond-scale radio pulses. Explici…

astro-ph.IM2025

End-to-end reconstruction of ultra-high energy particle observables from radio detection of extensive air showers

Kewen Zhang, Duan Kaikai, Ramesh Koirala +3

The radio detection of very inclined air showers offers a promising avenue for studying ultra-high-energy cosmic rays (UHECRs) and neutrinos. Accurate reconstruction methods are es…

astro-ph.IM2025

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025)

Jaime Álvarez-Muñiz, Rafael Alves Batista, Aurélien Benoit-Lévy +133

The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses la…

astro-ph.IM2025

Electric-Field Reconstruction for Radio Detection of Inclined Air Showers in Three Polarizations

Kewen Zhang, Lukas Gülzow, Tim Huege +7

Accurate reconstruction of the electric field produced by extensive air showers is essential for the radio-detection technique, as the key parameters of interest of the primary par…

astro-ph.HE2025

Analytical description of the radio Cherenkov cone

Valentin Decoene, Marion Guelfand, Matìas Tueros

Radio emissions from extensive air showers (EAS) provide a valuable tool for detecting ultra-high-energy (UHE) astroparticles. In this context, several radio arrays focus on detect…

astro-ph.HE2025

Reconstruction of inclined extensive air showers using radio signals: from arrival times and amplitudes to direction and energy

Marion Guelfand, Valentin Decoene, Olivier Martineau-Huynh +4

Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above eV. The next-generation of radio experiments…

astro-ph.HE2025

Uncertainties in the Estimation of Air Shower Observables from Monte Carlo Simulation of Radio Emission

Carlo S. Cruz Sanchez, Patricia M. Hansen, Matias Tueros +2

The detection of extensive air showers (EAS) induced by cosmic rays via radio signals has undergone significant advancements in the last two decades. Numerous ultra-high energy cos…

astro-ph.IM2020★ 5 cited

Synthesis of radio signals from extensive air showers using previously computed microscopic simulations

Matias Tueros, Anne Zilles

The detection of extensive air showers (EAS) through their radio signal is becoming one of the most promising techniques for the study of Neutrinos and Cosmic rays at the highest e…

astro-ph.IM2018★ 5 cited

Towards online triggering for the radio detection of air showers using deep neural networks

Florian Führer, Tom Charnock, Anne Zilles +1

The detection of air-shower events via radio signals requires to develop a trigger algorithm for a clean discrimination between signal and background events in order to reduce the…

astro-ph.IM2009

Discarded low energy particles in extensive air shower simulations: Effect on the shower Missing and Invisible Energy

M. J. Tueros

The energy carried away by neutral particles in ultra high energy cosmic ray showers can not be detected by fluorescence detectors. This energy is usually referred to as the "invis…

astro-ph.IM2009

Discarded low energy particles in extensive air shower simulations: Effect on the shower Energy Deposit

M. J. Tueros

The simulation of particle cascades initiated in the atmosphere by ultra high energy cosmic ray particles involves the generation and propagation of a huge amount of particles. As…