activity
19942026
most citedMeasurement of the J/Psi Meson and b-Hadron Production Cross Sections in ppbar Collisions at sqrt s = 1960 GeV

699 citations · 3.4k across the 107 of their papers we have counts for

collaborators

109 papers

astro-ph.IM2026

The beamformed trigger of RNO-G: its design and in-field performance

G Collaboration, S. Agarwal, J. A. Aguilar +76

The Radio Neutrino Observatory in Greenland (RNO-G) is a neutrino detector under construction at Summit Station, with 8 out of a planned 35 stations currently deployed. We have des…

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…

astro-ph.HE2025

Validating the performance of the Radio Neutrino Observatory in Greenland using cosmic-ray air showers

S. Agarwal, J. A. Aguilar, N. Alden +79

The Radio Neutrino Observatory in Greenland (RNO-G) is currently under construction with the aim to detect neutrinos with energies beyond . A critical part o…

astro-ph.HE2025★ 4 cited

Observation of In-ice Askaryan Radiation from High-Energy Cosmic Rays

ARA Collaboration, N. Alden, S. Ali +74

We present the first experimental evidence for in-ice Askaryan radiation -- coherent charge-excess radio emission -- from high-energy particle cascades developing in the Antarctic…

astro-ph.HE2025

First Radio Neutrino & Cosmic Rays Astronomy Workshop in India

Mohammad Ful Hossain Seikh, Victor Grachev, Ilya Kravchenko +2

We summarize the motivation for (as well as the presentations from) the April, 2024 workshop held in India and focused on radiowave techniques for cosmic ray and neutrino detection…

astro-ph.HE2025

The IceCube-Gen2 Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC2025)

R. Abbasi, M. Ackermann, J. Adams +465

IceCube-Gen2 is a planned next-generation neutrino observatory at the South Pole that builds upon the successful design of IceCube. Integrating two complementary detection technolo…

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.IM2025

Probing the Firn Refractive Index Profile Using Antenna Response

S. Agarwal, J. A. Aguilar, N. Alden +70

The Radio Neutrino Observatory-Greenland (RNO-G, at Summit Station) experiment comprises an extensive fat-dipole antenna array deployed into ice boreholes over an eventual area of…

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★ 2 cited

Instrument design and performance of the first seven stations of RNO-G

S. Agarwal, J. A. Aguilar, N. Alden +78

The Radio Neutrino Observatory in Greenland (RNO-G) is the first in-ice radio array in the northern hemisphere for the detection of ultra-high energy neutrinos via the coherent rad…

astro-ph.HE2024

ARA-Next: a new DAQ and trigger architecture for the Askaryan Radio Array

Pawan Giri, Ilya Kravchenko, Patrick Allison +1

The Askaryan Radio Array (ARA) experiment aims to detect ultra-high-energy cosmic neutrinos (>10 PeV) using radio detection techniques. To enhance ARA's capabilities, a new RFSoC-b…

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.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.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…