most citedGalactic and Extragalactic Analysis of the Astrophysical Muon Neutrino Flux with 12.3 years of IceCube Track Data

14 citations · 45 across the 47 of their papers we have counts for

collaborators

47 papers

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.HE2025

Multi-Messenger Search for Neutrino and Gravitational-Wave Emissions from Binary Black Holes Near Active Galactic Nuclei

Leonardo Ricca, Matthias Vereecken, Christoph Raab +3

Binary black holes (BBHs) in the vicinity of Active Galactic Nuclei (AGNs) are particularly interesting systems from both a cosmological and astrophysical point of view. Matter and…

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…

hep-ex2025

The ANTARES detector: two decades of neutrino searches in the Mediterranean Sea

A. Albert, S. Alves, M. André +138

Interest for studying cosmic neutrinos using deep-sea detectors has increase after the discovery of a diffuse flux of cosmic neutrinos by the IceCube collaboration and the possibil…

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…

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.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★ 3 cited

tilepy: rapid tiling strategies in mid/small FoV observatories

Fabian Schüssler, Halim Ashkar, Mathieu de Bony de Lavergne +1

The challenges inherent to time-domain multi-messenger astronomy require strategic actions so that adapted, optimized follow-up observations are performed efficiently. In particula…

astro-ph.HE2023

A Two-Component Lateral Distribution Function for the Reconstruction of Air-Shower Events in IceTop

Mark Weyrauch, Dennis Soldin

The surface component of the IceCube Neutrino Observatory, IceTop, consists of an array of ice-Cherenkov tanks measuring the electromagnetic signal as well as low-energy ($\sim\rm{…

astro-ph.HE2023

Extending the IceCube search for neutrino point sources in the Northern sky with additional years of data

Chiara Bellenghi, Martin Ha Minh, Tomas Kontrimas +3

The IceCube Neutrino Observatory is a one-cubic-kilometer-sized neutrino telescope deployed deep in the Antarctic ice at the South Pole. One of IceCube's major goals is finding the…

astro-ph.HE2023

Extending SkyLLH software for neutrino point source analyses with 10 years of IceCube public data

Chiara Bellenghi, Martina Karl, Martin Wolf

Searching for the sources of high-energy cosmic particles requires sophisticated analysis techniques, frequently involving hypothesis tests with unbinned log-likelihood (LLH) funct…

astro-ph.HE2023★ 14 cited

Galactic and Extragalactic Analysis of the Astrophysical Muon Neutrino Flux with 12.3 years of IceCube Track Data

Philipp Fürst

The Ice Cube Neutrino Observatory has been measuring an isotropic astrophysical neutrino flux in multiple detection channels for almost a decade. Galactic diffuse emission, which a…

astro-ph.HE2023★ 1 cited

Search for Extremely High Energy Neutrinos with IceCube

Maximilian Meier, Brian Clark

Extremely high energy (EHE) neutrinos (with energies above GeV) are produced in interactions of the highest energy cosmic rays. A primary contribution to the EHE neutrino fl…

astro-ph.IM2023

Operations plans and sensitivities of the IceCube Upgrade Camera System

Steven Rodan, Christoph Tönnis, Jiwoong Lee +1

The IceCube Upgrade consists of seven new strings to be deployed in the central region of the existing IceCube detector. The goals of the IceCube Upgrade are two-fold: to enhance s…

astro-ph.HE2023★ 1 cited

Indirect dark matter search in the Galactic Centre with IceCube

Nhan Chau, Juan A. Aguilar

It is assumed that dark matter can annihilate or decay into Standard Model particles which then can produce a neutrino flux detectable at IceCube. Such a signal can be emitted from…

astro-ph.IM2023★ 1 cited

A new simulation framework for IceCube Upgrade calibration using IceCube Upgrade Camera system

Christoph Tönnis, Seowon Choi, Carsten Rott +2

Currently, an upgrade consisting of seven densely instrumented strings in the center of the volume of the IceCube detector with new digital optical modules (DOMs) is being built. O…

astro-ph.HE2023

Refining the IceCube detector geometry using muon and LED calibration data

Matti Janson, Saskia Philippen, Martin Rongen

The IceCube Neutrino Observatory deployed 5160 digital optical modules (DOMs) on 86 cables, called strings, in a cubic kilometer of deep glacial ice below the geographic South Pole…

astro-ph.HE2023

Search for the rare interactions of neutrinos from distant point sources with IceCube Neutrino Telescope

Woosik Kang, Carsten Rott

The recent discovery and evidence of neutrino signals from distant sources, TXS 0506+056 and NGC 1068 respectively, provide opportunities to search for rare interactions of neutrin…

astro-ph.HE2023★ 1 cited

Search for Dark Matter Decay in Nearby Galaxy Clusters and Galaxies with IceCube

Minjin Jeong, Carsten Rott

Dark matter could decay into Standard Model particles producing neutrinos directly or indirectly. The resulting flux of neutrinos from these decays could be detectable at neutrino…