O. Martineau‐Huynh
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View article: Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes
Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes Open
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 long-sought origin of UHE cosmic rays by detecting large num…
View article: The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project Open
View article: The Giant Radio Array for Neutrino Detection - experimental status and plans
The Giant Radio Array for Neutrino Detection - experimental status and plans Open
View article: Reconstruction of inclined cosmic ray properties with GRAND data
Reconstruction of inclined cosmic ray properties with GRAND data Open
International audience
View article: Optimizing HERON for 100 PeV Neutrino Detection
Optimizing HERON for 100 PeV Neutrino Detection Open
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) is designed to target the astrophysical flux of Earth-skimming tau neutrinos at 100 PeV. HERON consists of multiple compact, phased radio arrays embedded within a larger sparse ar…
View article: The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025)
The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025) Open
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 large surface arrays of antennas to look for the radio emissi…
View article: Reconstruction of inclined cosmic-ray properties with GRAND data
Reconstruction of inclined cosmic-ray properties with GRAND data Open
Radio-detection is now an established technique for studying ultra-high-energy (UHE) cosmic rays with energies exceeding $\sim 10^{17}$ eV. The next generation of radio experiments, such as the Giant Radio Array for Neutrino Detection (GRA…
View article: The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project Open
Measuring ultra-high energy neutrinos, with energies above $10^{16}$ eV, is the next frontier of the emerging multi-messenger era. Their detection requires building a large-scale detector with 10 times the instantaneous sensitivity of curr…
View article: Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy Open
View article: Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy Open
Detecting ultrahigh-energy neutrinos can take two complementary approaches with different trade-offs. 1)~Wide and shallow: aim for the largest effective volume, and to be cost-effective, go for wide field-of-view but at the cost of a shall…
View article: Reconstruction of highly inclined extensive air showers in GRAND
Reconstruction of highly inclined extensive air showers in GRAND Open
International audience
View article: Development of an Autonomous Detection-Unit Self-Trigger for GRAND
Development of an Autonomous Detection-Unit Self-Trigger for GRAND Open
International audience
View article: Next-Generation Triggering: A Novel Event-Level Approach
Next-Generation Triggering: A Novel Event-Level Approach Open
Large-scale cosmic-ray detectors like the Giant Radio Array for Neutrino Detection (GRAND) are pushing the boundaries of our ability to identify air shower events. Existing trigger schemes rely solely on the timing of signals detected by i…
View article: 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)
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) Open
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 Detection Activities (ARENA 2024, University of Chicago, June…
View article: Development of an Autonomous Detection-Unit Self-Trigger for GRAND
Development of an Autonomous Detection-Unit Self-Trigger for GRAND Open
One of the major challenges for the radio detection of extensive air showers, as encountered by the Giant Radio Array for Neutrino Detection (GRAND), is the requirement of an autonomous radio self-trigger. This work presents the current de…
View article: Reconstruction of highly inclined extensive air showers in GRAND
Reconstruction of highly inclined extensive air showers in GRAND Open
The Giant Radio Array for Neutrino Detection (GRAND) aims to detect highly inclined extensive air showers (EAS) with down-going and up-going trajectories. Several working groups in the GRAND collaboration are developing methods to reconstr…
View article: Grandlib: A Simulation Pipeline for the Giant Radio Array for Neutrino Detection (Grand)
Grandlib: A Simulation Pipeline for the Giant Radio Array for Neutrino Detection (Grand) Open
View article: Snowmass UHECR Whitepaper: Requirements on Future Instrumentation
Snowmass UHECR Whitepaper: Requirements on Future Instrumentation Open
Complementing the overview contribution about the whitepaper on ultra-high-energy cosmic rays (UHECR) prepared for the Snowmass community survey in the U.S. [Astroparticle Physics 149 (2023) 102819 - arXiv:2205.05845], this contribution fo…
View article: “Ultra-High-Energy Cosmic-Rays (UHECR): at the Intersection of the Cosmic and Energy Frontiers” -- Overview of the Snowmass UHECR white paper and roadmap
“Ultra-High-Energy Cosmic-Rays (UHECR): at the Intersection of the Cosmic and Energy Frontiers” -- Overview of the Snowmass UHECR white paper and roadmap Open
As part of the US "Snowmass" community planning exercise, the UHECR community has come together to write a comprehensive white paper discussing the recent progress and open questions of the field, as they relate to the overarching goals of…
View article: The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)
The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023) Open
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 large surface arrays of autonomous radio-detection units to l…
View article: The Giant Radio Array for Neutrino Detection
The Giant Radio Array for Neutrino Detection Open
Ultra-high-energy cosmic neutrinos (UHE), with energies above 100 PeV, are unparalleled probes of the most energetic astrophysical sources and weak interactions at energies beyond the reach of accelerators. GRAND is an envisioned observato…
View article: A neural network to classify GRAND radio time traces
A neural network to classify GRAND radio time traces Open
GRAND is a Ultra High Energy (UHE) cosmic particles detection project, consisting in a giant,\nself-triggered, antenna array. Wherever we decide to setup the antennas apart from polar areas,\nwe will generally face a high rate of backgroun…
View article: Ultra high energy cosmic rays The intersection of the Cosmic and Energy Frontiers
Ultra high energy cosmic rays The intersection of the Cosmic and Energy Frontiers Open
View article: Publisher's Note:
Publisher's Note: Open
View article: Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays
Radio wavefront of very inclined extensive air-showers: A simulation study for extended and sparse radio arrays Open
View article: Polarisation signatures in radio for inclined cosmic-ray induced air-shower identification
Polarisation signatures in radio for inclined cosmic-ray induced air-shower identification Open
View article: Radio-Morphing: a fast, efficient and accurate tool to compute the radio signals from air-showers
Radio-Morphing: a fast, efficient and accurate tool to compute the radio signals from air-showers Open
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 needed to evaluate the radio signal at each antenna position…
View article: The Large High Altitude Air Shower Observatory (LHAASO) Science Book \n (2021 Edition)
The Large High Altitude Air Shower Observatory (LHAASO) Science Book
\n (2021 Edition) Open
Since the science white paper of the Large High Altitude Air Shower
\nObservatory (LHAASO) published on arXiv in 2019 [e-Print: 1905.02773
\n(astro-ph.HE)], LHAASO has completed the transition from a project to an
\noperational gamma-ray a…
View article: Chapter 4 Cosmic-Ray Physics *
Chapter 4 Cosmic-Ray Physics * Open
In the first part of this Chapter the present state of knowledge from the observations of cosmic rays between 10 13 and 10 20 eV is summarized. This is not intended to be a complete review, but rather a broad overview of the relevant proce…
View article: The path towards the Giant Radio Array for Neutrino Detection
The path towards the Giant Radio Array for Neutrino Detection Open