papers

Publications (17)

astro-ph.IM2024

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2024)

Rafael Alves Batista, Aurélien Benoit-Lévy, Teresa Bister +121

This is an index of the contributions by the Giant Radio Array for Neutrino Detection (GRAND) Collaboration to the 10th International Workshop on Acoustic and Radio EeV Neutrino De…

astro-ph.IM2021

A reconstruction procedure for near horizon extensive air showers based on radio signals

Valentin Decoene, Olivier Martineau-Huynh, Matìas Tueros +1

Very inclined extensive air showers (EAS), with both down-going and up-going trajectories, are particularly targeted by the next generation of extended radio arrays, such as GRAND.…

astro-ph.HE2024

Loss of coherence and change in emission physics for radio emission from very inclined cosmic-ray air showers

Simon Chiche, Chao Zhang, Felix Schlüter +5

Next-generation radio experiments such as the Radio Detector of the upgraded Pierre Auger Observatory and the planned GRAND and BEACON arrays target the detection of ultra-high-ene…

astro-ph.HE2022

Overview of radio experiments for UHE cosmic particles detection

Simon Chiche, Valentin Decoene

Radio-detection is a mature technique that has gained large momentum over the past decades. Its physical detection principle is mainly driven by the electromagnetic part of the sho…

astro-ph.IM2026

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.IM2024

GRANDlib: A simulation pipeline for the Giant Radio Array for Neutrino Detection (GRAND)

GRAND Collaboration, Rafael Alves Batista, Aurélien Benoit-Lévy +112

The operation of upcoming ultra-high-energy cosmic-ray, gamma-ray, and neutrino radio-detection experiments, like the Giant Radio Array for Neutrino Detection (GRAND), poses signif…

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.HE2022

Polarisation signatures in radio for inclined cosmic-ray induced air-shower identification

Simon Chiche, Kumiko Kotera, Olivier Martineau-Huynh +2

Autonomous radio-detection, i.e., detection of air-showers with standalone radio arrays, is one of the major technical challenges to overcome for the next generation astroparticle…

astro-ph.HE2024

Particle content of very inclined air showers for radio signal modeling

Marion Guelfand, Simon Chiche, Kumiko Kotera +2

The reconstruction of very inclined air showers is a new challenge for next-generation radio experiments such as the AugerPrime radio upgrade, BEACON, and GRAND, which focus on the…

astro-ph.HE2026

Radio Signatures of Cosmic-Ray Particle Showers in Deep In-Ice Antennas

Simon Chiche, Krijn D. de Vries, Simona Toscano

To detect ultra-high-energy neutrinos, experiments such as ARA and RNO-G target the radio emission induced by these particles as they cascade in the ice, using deep in-ice antennas…

hep-ex2024

The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)

GRAND Collaboration, Rafael Alves Batista, Aurélien Benoit-Lévy +96

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.HE2024

GRANDProto300: status, science case, and prospects

Simon Chiche

GRANDProto300, the mid-scale prototype of the GRAND experiment, is a planned radio array of 300 antennas over that will be deployed in the radio-quiet location o…

astro-ph.IM2022

Radio-Morphing: a fast, efficient and accurate tool to compute the radio signals from air-showers

Simon Chiche, Olivier Martineau-Huynh, Kumiko Kotera +2

Radio detection of air-showers is a mature technique that has gained momentum over the past decades. With increasingly large-scale experiments, massive air-shower simulations are n…

astro-ph.HE2024

Radio signatures of cosmic-ray showers with deep in-ice antennas

Simon Chiche, Nicolas Moller, Abby Bishop +4

To detect ultra-high-energy neutrinos, experiments such as ARA and RNO-G target the radio emission these particles induce when cascading in the ice, using deep antennas in South Po…

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.HE2026

In-ice Radio Signatures of Cosmic Ray Particle Cascades

Simon Chiche, Simona Toscano, Krijn D. de Vries

To detect ultra-high-energy neutrinos, experiments such as the Askaryan Radio Array and the Radio Neutrino Observatory in Greenland target the radio emission induced by these parti…

astro-ph.GA2021

Jellyfish galaxy candidates in MACS J0717.5+3745 and thirty-nine other clusters of the DAFT/FADA and CLASH surveys

Florence Durret, Simon Chiche, Catarina Lobo +1

Galaxies in clusters undergo several phenomena such as ram pressure stripping and tidal interactions, that can trigger or quench their star formation and, in some cases, lead to ga…