collaborators

5 papers

astro-ph.HE2026

Simulation of combined radio and radar signals at the Radar Echo Telescope for Cosmic Rays

K. Nivedita, I. Loudon, J. Loonen +29

To explore neutrino astronomy at high energies (> 10 PeV), the Radar Echo Telescope for Cosmic Rays (RET-CR) was developed to assess the feasibility of a radar technique for detect…

astro-ph.IM2026

Trigger system for the Payload for Ultrahigh Energy Observations (PUEO) balloon-borne neutrino detector

Q. Abarr, J. Alfaro, P. Allison +67

The Payload for Ultrahigh Energy Observations (PUEO) is a NASA balloon-borne instrument for the detection of ultra-high energy (UHE) neutrinos with energies above $10^{17.5}~\textr…

astro-ph.HE2026

Seasonal Variation of Polar Ice: Implications for Ultrahigh Energy Neutrino Detectors

Alexander Kyriacou, Steven Prohira, Dave Besson

The upper to of the polar ice sheet, called the firn, has a time-dependent density due to seasonal variations in the surface temperature and…

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

Sensitivity of BEACON to Ultra-High Energy Diffuse and Transient Neutrinos

Andrew Zeolla, Jaime Alvarez-Muñiz, Sergio Cabana-Freire +16

Ultra-high energy neutrinos ( eV) can provide insight into the most powerful accelerators in the universe, however their flux is extremely low. The Beamforming Elevated…