activity
20162025
most citedNeutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

1.1k citations · 2.5k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2025★ 1 cited

Prompt Searches for Very-High-Energy γ-Ray Counterparts to IceCube Astrophysical Neutrino Alerts

J. Abhir, A. Biland, K. Brand +817

The search for sources of high-energy astrophysical neutrinos can be significantly advanced through a multi-messenger approach, which seeks to detect the gamma rays that accompany…

astro-ph.HE2025★ 1 cited

Enhancing air-shower observations: Results from an IceCube Surface Array Prototype Station

Megha Venugopal

The Surface Array Enhancement of the IceCube Neutrino Observatory is set to equip the existing surface cosmic-ray array of ice-Cherenkov detectors, IceTop, with radio antennas and…

astro-ph.HE2022★ 26 cited

Search for Astrophysical Neutrinos from 1FLE Blazars with IceCube

R. Abbasi, M. Ackermann, J. Adams +379

The majority of astrophysical neutrinos have undetermined origins. The IceCube Neutrino Observatory has observed astrophysical neutrinos but has not yet identified their sources. B…

hep-ex2022★ 20 cited

Low Energy Event Reconstruction in IceCube DeepCore

R. Abbasi, M. Ackermann, J. Adams +381

The reconstruction of event-level information, such as the direction or energy of a neutrino interacting in IceCube DeepCore, is a crucial ingredient to many physics analyses. Algo…

astro-ph.HE2021★ 241 cited

Improved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data

R. Abbasi, M. Ackermann, J. Adams +376

We present a measurement of the high-energy astrophysical muon-neutrino flux with the IceCube Neutrino Observatory. The measurement uses a high-purity selection of ~650k neutrino-i…

astro-ph.HE2021★ 46 cited

A search for neutrino emission from cores of Active Galactic Nuclei

R. Abbasi, M. Ackermann, J. Adams +376

The sources of the majority of the high-energy astrophysical neutrinos observed with the IceCube neutrino telescope at the South Pole are unknown. So far, only a gamma-ray blazar w…

astro-ph.HE2021★ 28 cited

Search for multi-flare neutrino emissions in 10 years of IceCube data from a catalog of sources

IceCube collaboration, R. Abbasi, M. Ackermann +375

A recent time-integrated analysis of a catalog of 110 candidate neutrino sources revealed a cumulative neutrino excess in the data collected by IceCube between April 6, 2008 and Ju…

astro-ph.HE2021★ 18 cited

Combining Maximum-Likelihood with Deep Learning for Event Reconstruction in IceCube

Mirco Hünnefeld

The field of deep learning has become increasingly important for particle physics experiments, yielding a multitude of advances, predominantly in event classification and reconstru…

astro-ph.HE2021★ 5 cited

Reconstructing Neutrino Energy using CNNs for GeV Scale IceCube Events

Jessie Micallef

Measurements of neutrinos at and below 10 GeV provide unique constraints of neutrino oscillation parameters as well as probes of potential Non-Standard Interactions (NSI). The IceC…

astro-ph.HE2021★ 10 cited

Study of Mass Composition of Cosmic Rays with IceTop and IceCube

Paras Koundal, Matthias Plum, Julian Saffer

The IceCube Neutrino Observatory is a multi-component detector at the South Pole which detects high-energy particles emerging from astrophysical events. These particles provide us…

astro-ph.HE2021★ 11 cited

Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory

IceCube Collaboration, R. Abbasi, M. Ackermann +415

The advent of multi-messenger astronomy has allowed for new types of source searches by neutrino detectors. We present the results of the search for 0.5-100 GeV astrophysical neutr…

astro-ph.IM2021★ 82 cited

Supernova Model Discrimination with Hyper-Kamiokande

Kamiokande Collaboration, K. Abe, P. Adrich +499

Core-collapse supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants…

astro-ph.HE2021★ 15 cited

Search for GeV Neutrino Emission During Intense Gamma-Ray Solar Flares with the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +364

Solar flares convert magnetic energy into thermal and non-thermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injecte…

astro-ph.HE2020★ 20 cited

A search for time-dependent astrophysical neutrino emission with IceCube data from 2012 to 2017

IceCube Collaboration, R. Abbasi, M. Ackermann +361

High-energy neutrinos are unique messengers of the high-energy universe, tracing the processes of cosmic-ray acceleration. This paper presents analyses focusing on time-dependent n…

astro-ph.HE2020★ 19 cited

Measurements of the Time-Dependent Cosmic-Ray Sun Shadow with Seven Years of IceCube Data -- Comparison with the Solar Cycle and Magnetic Field Models

M. G. Aartsen, R. Abbasi, M. Ackermann +376

Observations of the time-dependent cosmic-ray Sun shadow have been proven as a valuable diagnostic for the assessment of solar magnetic field models. In this paper, seven years of…

astro-ph.HE2020★ 38 cited

Cosmic Ray Spectrum from 250 TeV to 10 PeV using IceTop

IceCube Collaboration

We report here an extension of the measurement of the all-particle cosmic-ray spectrum with IceTop to lower energy. The new measurement gives full coverage of the knee region of th…

physics.ins-det2020★ 32 cited

In-situ calibration of the single-photoelectron charge response of the IceCube photomultiplier tubes

The IceCube Collaboration

We describe an improved in-situ calibration of the single-photoelectron charge distributions for each of the in-ice Hamamatsu Photonics R7081-02[MOD] photomultiplier tubes in the I…

hep-ex2019★ 53 cited

Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

Gen2 Collaboration, M. G. Aartsen, M. Ackermann +440

The ordering of the neutrino mass eigenstates is one of the fundamental open questions in neutrino physics. While current-generation neutrino oscillation experiments are able to pr…

astro-ph.HE2019★ 450 cited

Time-integrated Neutrino Source Searches with 10 years of IceCube Data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +357

This paper presents the results from point-like neutrino source searches using ten years of IceCube data collected between Apr.~6, 2008 and Jul.~10, 2018. We evaluate the significa…

hep-ex2019★ 43 cited

Efficient propagation of systematic uncertainties from calibration to analysis with the SnowStorm method in IceCube

M. G. Aartsen, M. Ackermann, J. Adams +357

Efficient treatment of systematic uncertainties that depend on a large number of nuisance parameters is a persistent difficulty in particle physics experiments. Where low-level eff…

astro-ph.HE2019★ 165 cited

Cosmic Ray Spectrum and Composition from PeV to EeV Using 3 Years of Data From IceTop and IceCube

IceCube Collaboration

We report on measurements of the all-particle cosmic ray energy spectrum and composition in the PeV to EeV energy range using three years of data from the IceCube Neutrino Observat…

astro-ph.HE2018★ 1.1k cited

Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

IceCube Collaboration

A high-energy neutrino event detected by IceCube on 22 September 2017 was coincident in direction and time with a gamma-ray flare from the blazar TXS 0506+056. Prompted by this ass…

hep-ex2016★ 108 cited

Physics Potentials with the Second Hyper-Kamiokande Detector in Korea

Hyper-Kamiokande proto-collaboration, :, K. Abe +353

Hyper-Kamiokande consists of two identical water-Cherenkov detectors of total 520~kt with the first one in Japan at 295~km from the J-PARC neutrino beam with 2.5 Off…