activity
20212025
most citedA next-generation optical sensor for IceCube-Gen2

4 citations · 7 across the 14 of their papers we have counts for

collaborators

16 papers

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★ 2 cited

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…

astro-ph.IM2024★ 1 cited

MAUVE: An Ultraviolet Astrophysics Probe Mission Concept

Mayura Balakrishnan, Rory Bowens, Fernando Cruz Aguirre +18

We present the mission concept "Mission to Analyze the UltraViolet universE" (MAUVE), a wide-field spectrometer and imager conceived during the inaugural NASA Astrophysics Mission…

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.IM2024

Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas

Stephanie Wissel, Andrew Zeolla, Cosmin Deaconu +20

Neutrinos at ultrahigh energies can originate both from interactions of cosmic rays at their acceleration sites and through cosmic-ray interactions as they propagate through the un…

astro-ph.HE2023

Sensitivity of IceCube-Gen2 to measure flavor composition of Astrophysical neutrinos

Neha Lad

The observation of an astrophysical neutrino flux in IceCube and its detection capability to separate between the different neutrino flavors has led IceCube to constraint the flavo…

astro-ph.IM2023

Mechanical design of the optical modules intended for IceCube-Gen2

Yuya Makino

IceCube-Gen2 is an expansion of the IceCube neutrino observatory at the South Pole that aims to increase the sensitivity to high-energy neutrinos by an order of magnitude. To this…

astro-ph.HE2023

The next generation neutrino telescope: IceCube-Gen2

Aya Ishihara

The IceCube Neutrino Observatory, a cubic-kilometer-scale neutrino detector at the geographic South Pole, has reached a number of milestones in the field of neutrino astrophysics:…

astro-ph.HE2023

Performance Studies of the Acoustic Module for the IceCube Upgrade

Charlotte Benning, Jürgen Borowka, Christoph Günther +2

The IceCube Upgrade will augment the existing IceCube Neutrino Observatory by deploying 700 additional optical sensor modules and calibration devices within its center at a depth o…

astro-ph.HE2023

The Surface Array of IceCube-Gen2

Alan Coleman

The science goals of IceCube-Gen2 include multi-messenger astronomy, astroparticle and particle physics. To this end, the observatory will include several detection methods, includ…

astro-ph.IM2023

Electronics Design of the IceCube-Gen2 Optical Module Prototype

Sean Griffin

IceCube-Gen2 is a planned extension to the existing IceCube Neutrino Observatory and will provide an order of magnitude increase in the detection rate of cosmic neutrinos by deploy…

astro-ph.HE2023

Estimating the coincidence rate between the optical and radio array of IceCube-Gen2

Felix Schlüter, Simona Toscano

The IceCube-Gen2 Neutrino Observatory is proposed to extend the all-flavour energy range of IceCube beyond PeV energies. It will comprise two key components: I) An enlarged 8km…

astro-ph.HE2023

Sensitivity of the IceCube-Gen2 Surface Array for Cosmic-Ray Anisotropy Studies

Wenjie Hou

The energy of the transition from Galactic to extra-galactic origin of cosmic rays is one of the major unresolved issues of cosmic-ray physics. However, strong constraints can be o…

astro-ph.IM2023

Performance studies on new 4" photomultiplier types intended for IceCube-Gen2 optical modules

Markus Dittmer, Alexander Kappes

In the upcoming IceCube-Gen2 extension, the newly developed optical modules will include 4-inch PMTs. For this purpose, the manufacturers Hamamatsu and North Night Vision Technolog…

physics.ins-det2022

Radiofrequency Ice Dielectric Measurements at Summit Station, Greenland

J. A. Aguilar, P. Allison, D. Besson +65

We recently reported on the radio-frequency attenuation length of cold polar ice at Summit Station, Greenland, based on bistatic radar measurements of radio-frequency bedrock echo…

astro-ph.IM2021★ 4 cited

A next-generation optical sensor for IceCube-Gen2

Vedant Basu, Aya Ishihara, Markus Dittmer +1

For the in-ice component of the next generation neutrino observatory at the South Pole, IceCube-Gen2, a new sensor module is being developed, which is an evolution of the D-Egg and…