activity
20132026
most citedLarge-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory

133 citations · 306 across the 96 of their papers we have counts for

collaborators

96 papers

astro-ph.IM2026

CORSIKA 8: A General Framework for Particle Cascade Simulations

J. M. Alameddine, J. Albrecht, A. A Alves +34

The simulation of extensive air showers and particle cascades in general is a cornerstone of modern astroparticle physics. For more than two decades, CORSIKA, currently in version…

astro-ph.HE2025

Constraints on the Population of Common Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of the LIGO and Virgo Detectors

Doğa Veske, Zsuzsa Márka, Albert Zhang

The discovery of joint sources of high-energy neutrinos and gravitational waves has been a primary target for the LIGO, Virgo, KAGRA, and IceCube observatories. The joint detection…

astro-ph.HE2025

Towards the Composition of sub-PeV Cosmic Rays at IceCube

Julian Saffer

With the implementation of a low-energy trigger, the surface array of the IceCube Neutrino Observatory is able to record cosmic-ray induced air showers with a primary energy of a f…

astro-ph.IM2025

Likelihood Reconstruction for Radio Detectors of Neutrinos and Cosmic Rays

Martin Ravn, Christian Glaser, Thorsten Glüsenkamp +2

Ultra-high-energy neutrinos and cosmic rays are excellent probes of astroparticle physics phenomena. For astroparticle physics analyses, robust and accurate reconstruction of signa…

astro-ph.HE2025

Probing neutrino emission at GeV energies from compact binary mergers detected during O1-O4a with the IceCube Neutrino Observatory

Karlijn Kruiswijk, Mathieu Lamoureux, Matthias Vereecken +1

Compact binary mergers, detected in gravitational waves since 2015, are candidate sources for astrophysical neutrinos in the GeV regime from proton-proton and proton-neutron collis…

astro-ph.HE2025

Measurement of the Three-Flavor Composition of Astrophysical Neutrinos with Contained IceCube Events

Aswathi Balagopal V., Vedant Basu, Albrecht Karle

The IceCube Neutrino Observatory at the South Pole detects neutrinos from the entire sky, both of astrophysical and atmospheric origin, via the Cherenkov light emitted when these n…

astro-ph.HE2025

Results from IceCube Follow-up of Nearby Supernova SN2023ixf

Alicia Mand, Justin Vandenbroucke, Jessie Thwaites +2

Core-collapse supernovae are of particular interest in multi-messenger astronomy due to their potential to accelerate cosmic rays and produce high-energy neutrinos. One such supern…

astro-ph.HE2025★ 2 cited

Measurement of the Diffuse Astrophysical Neutrino Spectrum above a TeV with All Flavor Starting Events in IceCube

Vedant Basu, Aswathi Balagopal V., Albrecht Karle

The IceCube Neutrino Observatory utilizes the Cherenkov radiation emitted by charged secondary particles produced in interactions of neutrinos with ice nucleons to detect neutrino…

astro-ph.HE2025

Cosmic Ray Detection with the IceTop Enhancement

Megha Venugopal

IceTop is the cosmic-ray detector located on the surface of the IceCube Neutrino Observatory at the South Pole, consisting of 81 pairs of ice-Cherenkov tanks. The rise in the energ…

astro-ph.HE2025

Plans for a new array of radio antennas for the detection of air showers at the 433m surface-detector array of the Pierre Auger Observatory

Stef Verpoest, Frank Schroeder, Alexander Novikov +6

We present the design and science case for a new array of radio antennas to be located at the Pierre Auger Observatory. Six stations of three SKALA antennas each will be deployed a…

astro-ph.IM2025

Ideas and Requirements for the Global Cosmic-Ray Observatory (GCOS)

Markus Ahlers, Ingo Allekotte, Jaime Alvarez-Muniz +136

After a successful kick-off meeting in 2021. two workshops in 2022 and 2023 on the future Global Cosmic-Ray Observatory (GCOS) focused mainly on a straw man design of the detector…

astro-ph.HE2024★ 3 cited

In-ice Askaryan Emission from Air Showers: Implications for Radio Neutrino Detectors

Alan Coleman, Christian Glaser, Ryan Rice-Smith +2

One of the most promising techniques for detecting ultra-high energy neutrinos involves the use of radio antennas to observe the 10-1000 MHz radiation generated by the showers that…

astro-ph.IM2024

Likelihood reconstruction of radio signals of neutrinos and cosmic rays

Martin Ravn, Christian Glaser, Thorsten Glüsenkamp +1

Ultra-high-energy neutrinos and cosmic rays are excellent probes of astroparticle physics phenomena. For astroparticle physics analyses, robust and accurate reconstruction of signa…

astro-ph.IM2024

Status and plans for the instrumentation of the IceCube Surface Array Enhancement

S. Shefali, Frank G. Schroeder

The surface array of IceCube, IceTop, operates primarily as a cosmic-ray detector, as well as a veto for astrophysical neutrino searches for the IceCube in-ice instrumentation. How…

astro-ph.HE2024★ 10 cited

The flavor composition of ultra-high-energy cosmic neutrinos: measurement forecasts for in-ice radio-based EeV neutrino telescopes

Alan Coleman, Oscar Ericsson, Mauricio Bustamante +1

In-ice radio-detection is a promising technique to discover and characterize ultra-high-energy (UHE) neutrinos, with energies above 100 PeV, adopted by present - ARA, ARIANNA, and…

astro-ph.HE2023

Simulating radio emission from air showers with CORSIKA 8

Nikolaos Karastathis, Remy Prechelt, Juan Ammerman-Yebra +2

CORSIKA 8 is a new framework for air shower simulations implemented in modern C++17, based on past experience with existing codes like CORSIKA 7. The flexible and modular structure…

astro-ph.HE2023

Constraining MeV Neutrino Emission of Bright Transients with IceCube

Nora Valtonen-Mattila, Spencer Griswold, Segev BenZvi

MeV neutrinos are produced in many astrophysical transients, such as stellar collapses and high-energy jets, where they play a role in sustaining and cooling energetic explosions.…

astro-ph.HE2023

Conditional normalizing flows for IceCube event reconstruction

Thorsten Glüsenkamp

The IceCube Neutrino Observatory is a cubic-kilometer high-energy neutrino detector deployed in the Antarctic ice. Two major event classes are charged-current electron and muon neu…

astro-ph.HE2023★ 3 cited

Joint searches by FACT, H.E.S.S., MAGIC and VERITAS for VHE gamma-ray emission associated with neutrinos detected by IceCube

Fabian Schüssler, Halim Ashkar, Elisa Bernardini +11

The sources of the astrophysical flux of high-energy neutrinos detected by IceCube are still largely unknown, but searches for temporal and spatial correlation between neutrinos an…

physics.comp-ph2023★ 2 cited

Comparison and efficiency of GPU accelerated optical light propagation in CORSIKA 8

Dominik Baack, Jean-Marco Alameddine

AI accelerators have proliferated in data centers in recent years and are now almost ubiquitous. In addition, their computational power and, most importantly, their energy efficien…

astro-ph.HE2023

Search for the Prompt Atmospheric Neutrino Flux in IceCube

Jakob Böttcher

For about a decade the IceCube Neutrino Observatory has been observing a high-energy diffuse astrophysical neutrino flux. At these energies, an important source of background are t…

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

Searching for IceCube sub-TeV neutrino counterparts to sub-threshold Gravitational Wave events

Tista Mukherjee

Since the release of the Gravitational Wave Transient Catalogue GWTC-2.1 by the LIGO-Virgo collaboration, sub-threshold gravitational wave (GW) candidates are publicly available. T…

astro-ph.IM2023★ 4 cited

Parallel processing of radio signals and detector arrays in CORSIKA 8

A. Augusto Alves, Nikolaos Karastathis, Tim Huege

This contribution describes some recent advances in the parallelization of the generation and processing of radio signals emitted by particle showers in CORSIKA 8. CORSIKA 8 is a M…