activity
20142026
most citedObservation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

1.2k citations · 3.3k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2026

Search for Diffuse Supernova Neutrino Background in the Full KamLAND Dataset with Neural-Network-Based Event Classification

D. Chernyak, T. Eda, M. Eizuka +63

We report a search for the diffuse supernova neutrino background (DSNB) with the KamLAND detector, targeting electron antineutrinos via inverse beta decay in the neutrino energy ra…

nucl-ex2026

New limits on the Pauli forbidden transitions in 12C nuclei obtained with the complete Borexino dataset

Borexino collaboration, D. Basilico, G. Bellini +70

The Pauli exclusion principle (PEP) was tested for nucleons in nuclei using the Borexino dataset from 2007 to 2021. %the complete Borexino detector data. The approach…

hep-ex2026

Constraints on non-standard neutrino interactions from Borexino extended data-set

V. Antonelli, D. Basilico, G. Bellini +74

Neutrino non-standard interactions (NSI) constitute an active research field, as they are closely related to potential new physics associated with dark matter searches and exotic i…

physics.ins-det2025★ 1 cited

Innovating Bolometers' Mounting: A Gravity-Based Approach

The CUPID Collaboration, K. Alfonso, A. Armatol +190

Cryogenic calorimeters, also known as bolometers, are among the leading technologies for searching for rare events. The CUPID experiment is exploiting this technology to deploy a t…

physics.ins-det2025★ 18 cited

CUPID, the CUORE Upgrade with Particle IDentification

The CUPID Collaboration, K. Alfonso, A. Armatol +190

CUPID, the CUORE Upgrade with Particle IDentification, is a next-generation experiment to search for neutrinoless double beta decay () and other rare events using enriched Li…

astro-ph.HE2024

Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All Time

T. Araki, S. Chauhan, K. Chiba +69

The electron antinuetrino flux limits are presented for the brightest gamma-ray burst (GRB) of all time, GRB221009A, over a range of 1.8-200 MeV using the Kamioka Liquid Scintillat…

hep-ex2023★ 4 cited

Novel techniques for alpha/beta pulse shape discrimination in Borexino

D. Basilico, G. Bellini, J. Benziger +71

Borexino could efficiently distinguish between alpha and beta radiation in its liquid scintillator by the characteristic time profile of their scintillation pulse. This alpha/beta…

astro-ph.HE2023★ 7 cited

Borexino's search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database

BOREXINO Collaboration, D. Basilico, G. Bellini +72

The search for neutrino events in correlation with gravitational wave (GW) events for three observing runs (O1, O2 and O3) from 09/2015 to 03/2020 has been performed using the Bore…

physics.ins-det2021

The Low Polonium Field of Borexino and its significance for the CNO neutrino detection

S. Kumaran, M. Agostini, K. Altenmüller +93

Borexino is a liquid scintillator detector located at the Laboratori Nazionale del Gran Sasso, Italy with the main goal to measure solar neutrinos. The experiment recently provided…

physics.data-an2018

Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit

X. F. Ding, M. Agostini, K. Altenmuller +104

A spectral fitter based on the graphics processor unit (GPU) has been developed for Borexino solar neutrino analysis. It is able to shorten the fitting time to a superior level com…

astro-ph.HE2017★ 52 cited

Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube

A. Albert, M. Andre, M. Anghinolfi +1410

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up…

astro-ph.HE2017★ 51 cited

Multiwavelength follow-up of a rare IceCube neutrino multiplet

M. G. Aartsen, M. Ackermann, J. Adams +501

On February 17 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with comi…

hep-ex2017★ 152 cited

Search for sterile neutrino mixing using three years of IceCube DeepCore data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +305

We present a search for a light sterile neutrino using three years of atmospheric neutrino data from the DeepCore detector in the energy range of approximately GeV. DeepCor…

astro-ph.IM2016★ 823 cited

The IceCube Neutrino Observatory: Instrumentation and Online Systems

IceCube Collaboration, M. G. Aartsen, M. Ackermann +350

The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detect…

hep-ex2016★ 58 cited

Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube

IceCube Collaboration, M. G. Aartsen, K. Abraham +537

We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescope…

astro-ph.HE2016★ 270 cited

The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux

IceCube Collaboration, M. G. Aartsen, K. Abraham +319

The recent discovery of a diffuse cosmic neutrino flux extending up to PeV energies raises the question of which astrophysical sources generate this signal. One class of extragalac…

hep-ex2014★ 137 cited

Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +301

We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a regio…

astro-ph.HE2014★ 296 cited

Atmospheric and Astrophysical Neutrinos above 1 TeV Interacting in IceCube

M. G. Aartsen, M. Ackermann, J. Adams +301

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for ~TeV neu…

astro-ph.HE2014★ 50 cited

Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +300

Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of to the -scale. The origin of those events, b…

astro-ph.HE2014★ 1.2k cited

Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

M. G. Aartsen, M. Ackermann, J. Adams +294

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial ori…

astro-ph.HE2014★ 39 cited

Multimessenger Search for Sources of Gravitational Waves and High-Energy Neutrinos: Results for Initial LIGO-Virgo and IceCube

The IceCube Collaboration, The LIGO Scientific Collaboration, The Virgo Collaboration +1185

We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neu…

astro-ph.HE2014★ 195 cited

Searches for Extended and Point-like Neutrino Sources with Four Years of IceCube Data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +301

We present results on searches for point-like sources of neutrinos using four years of IceCube data, including the first year of data from the completed 86-string detector. The tot…