activity
20152022
most citedImproved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data

241 citations · 1.3k across the 27 of their papers we have counts for

collaborators

27 papers

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★ 9 cited

First Search for Unstable Sterile Neutrinos with the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +380

We present a search for an unstable sterile neutrino by looking for a matter-induced signal in eight years of atmospheric data collected from 2011 to 2019 at the IceCube Neut…

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…

hep-ex2021★ 41 cited

Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube

R. Abbasi, M. Ackermann, J. Adams +378

Along their long propagation from production to detection, neutrino states undergo quantum interference which converts their types, or flavours. High-energy astrophysical neutrinos…

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.IM2021★ 4 cited

A next-generation optical sensor for IceCube-Gen2

Vedant Basu, Aya Ishihara, Markus Dittmer +1

For the in-ice component of the next generation neutrino observatory at the South Pole, IceCube-Gen2, a new sensor module is being developed, which is an evolution of the D-Egg and…

astro-ph.HE2021★ 3 cited

Multi-messenger searches via IceCube's high-energy neutrinos and gravitational-wave detections of LIGO/Virgo

Doğa Veske, Raamis Hussain, Zsuzsa Márka +5

We summarize initial results for high-energy neutrino counterpart searches coinciding with gravitational-wave events in LIGO/Virgo's GWTC-2 catalog using IceCube's neutrino trigger…

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★ 17 cited

Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies with IceCube

IceCube Collaboration, R. Abbasi, M. Ackermann +378

Ultra-luminous infrared galaxies (ULIRGs) have infrared luminosities , making them the most luminous objects in the infrared sky. These dust…

hep-ex2021★ 1 cited

All-flavor constraints on nonstandard neutrino interactions and generalized matter potential with three years of IceCube DeepCore data

IceCube Collaboration, R. Abbasi, M. Ackermann +370

We report constraints on nonstandard neutrino interactions (NSI) from the observation of atmospheric neutrinos with IceCube, limiting all individual coupling strengths from a singl…

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…

hep-ex2020★ 47 cited

Detection of astrophysical tau neutrino candidates in IceCube

R. Abbasi, M. Ackermann, J. Adams +361

High-energy tau neutrinos are rarely produced in atmospheric cosmic-ray showers or at cosmic particle accelerators, but are expected to emerge during neutrino propagation over cosm…

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…

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.IM2017★ 10 cited

The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part VI: IceCube-Gen2, the Next Generation Neutrino Observatory

Gen2 Collaboration, M. G. Aartsen, M. Ackermann +356

Papers on research & development towards IceCube-Gen2, the next generation neutrino observatory at South Pole, submitted to the 35th International Cosmic Ray Conference (ICRC 2017,…

astro-ph.HE2017★ 15 cited

Measurement of the energy spectrum with IceCube-79

M. G. Aartsen, M. Ackermann, J. Adams +306

IceCube is a neutrino observatory deployed in the glacial ice at the geographic South Pole. The energy unfolding described in this paper is based on data taken with IceCube i…