activity
20192026
most citedDesign and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)

116 citations · 375 across the 35 of their papers we have counts for

collaborators

37 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.HE2026

Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos

ARA Collaboration, N. Alden, S. Ali +71

The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino observatory designed to detect the impulsive radio waves produced by relativistic particle cascades in the Ant…

hep-ex2025

Radio emission from airplanes as observed with RNO-G

G Collaboration, S. Agarwal, J. A. Aguilar +79

This paper describes how intentional and unintentional radio emission from airplanes is recorded with the Radio Neutrino Observatory Greenland (RNO-G). We characterize the received…

astro-ph.HE2024

Askaryan Radio Array: searching for the highest energy neutrinos

Mohammad Ful Hossain Seikh

Searches for ultra-high energy ( PeV) cosmogenic and astrophysical neutrinos (UHENs) have been conducted by several experiments over the last two decades. The Askaryan…

astro-ph.IM2024★ 1 cited

Modeling the refractive index profile n(z) of polar ice for ultra-high energy neutrino experiments

S. Ali, P. Allison, S. Archambault +67

We have developed an in-situ index of refraction profile n(z) for cold polar ice, using the transit times of radio signals broadcast from an englacial transmitter to 2-5 km distant…

astro-ph.SR2024★ 3 cited

Solar flare observations with the Radio Neutrino Observatory Greenland (RNO-G)

S. Agarwal, J. A. Aguilar, S. Ali +69

The Radio Neutrino Observatory - Greenland (RNO-G) seeks discovery of ultra-high energy neutrinos from the cosmos through their interactions in ice. The science program extends bey…

astro-ph.HE2024★ 9 cited

Simulation of radio signals from cosmic-ray cascades in air and ice as observed by in-ice Askaryan radio detectors

Simon De Kockere, Dieder Van den Broeck, Uzair Abdul Latif +4

A new generation of neutrino observatories will search for PeV-EeV neutrinos interacting in the ice by detecting radio pulses. Extended air showers propagating into the ice will fo…

astro-ph.HE2023

Macroscopic approach to the radar echo scatter from high-energy particle cascades

E. Huesca Santiago, K. D. de Vries, P. Allison +28

To probe the cosmic particle flux at the highest energies, large volumes of dense material like ice have to be monitored. This can be achieved by exploiting the radio signal. In th…

astro-ph.HE2023

VAE-based latent-space classification of RNO-G data

Thorsten Glüsenkamp

The Radio Neutrino Observatory in Greenland (RNO-G) is a radio-based ultra-high energy neutrino detector located at Summit Station, Greenland. It is still being constructed, with 7…

astro-ph.IM2023★ 4 cited

Simulations of cross media showers with CORSIKA 8

Juan Ammerman-Yebra, Uzair Abdul Latif, Nikolaos Karastathis +2

The CORSIKA 8 project aims to develop a versatile and modern framework for particle shower simulations that meets the new needs of experiments and addresses the caveats of existing…

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

Benefits of Looking for Coincident Events, Taus, and Muons with the Askaryan Radio Array

Abby Bishop, Austin Cummings, Ryan Krebs +1

Ultra-High Energy (UHE) neutrinos over eV have yet to be observed but the Askaryan Radio Array (ARA) is one in-ice neutrino observatory attempting to make this discovery.…

astro-ph.IM2023

Calibration and Physics with ARA Station 1: A Unique Askaryan Radio Array Detector

M. F. H Seikh, D. Z. Besson, S. Ali +70

The Askaryan Radio Array Station 1 (A1), the first among five autonomous stations deployed for the ARA experiment at the South Pole, is a unique ultra-high energy neutrino (UHEN) d…

astro-ph.HE2023★ 2 cited

Multimessenger Potential of the Radio Neutrino Observatory in Greenland

Marco Stein Muzio

The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ~PeV) neutrino monitor of the Northern sky and will soon be the world's most sen…

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

Deep Learning Based Event Reconstruction for the IceCube-Gen2 Radio Detector

Nils Heyer, Christian Glaser, Thorsten Glüsenkamp

The planned in-ice radio array of IceCube-Gen2 at the South Pole will provide unprecedented sensitivity to ultra-high-energy (UHE) neutrinos in the EeV range. The ability of the de…

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…

astro-ph.IM2023★ 2 cited

Precision measurement of the index of refraction of deep glacial ice at radio frequencies at Summit Station, Greenland

J. A. Aguilar, P. Allison, D. Besson +71

Glacial ice is used as a target material for the detection of ultra-high energy neutrinos, by measuring the radio signals that are emitted when those neutrinos interact in the ice.…