activity
20242026
collaborators

8 papers

astro-ph.IM2026

Short-Term Turbulence Prediction for Seeing Using Machine Learning

Mary Joe Medlej, Rahul Srinivasan, Simon Prunet +2

Optical turbulence, driven by fluctuations of the atmospheric refractive index, poses a significant challenge to ground-based optical systems, as it distorts the propagation of lig…

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.IM2025

Diffusion models for polarimetric reconstruction of circumstellar environments

Quentin Villegas, Laurence Denneulin, Simon Prunet +5

In this paper, we propose an approach combining diffusion models and inverse problems for the reconstruction of circumstellar disk images. Our method builds upon the Rhapsodie fram…

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.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.IM2025

Analytical planar wavefront reconstruction and error estimates for radio detection of extensive air showers

Arsène Ferrière, Simon Prunet, Aurélien Benoit-Lévy +3

When performing radio detection of ultra-high energy astroparticles, the planar wavefront model is often used as a first step to evaluate the arrival direction of primary particles…