activity
20082023
most citedThe IceCube Neutrino Observatory: Instrumentation and Online Systems

823 citations · 4.9k across the 42 of their papers we have counts for

collaborators

44 papers

physics.acc-ph2023

TEX (TEst stand for X-band) at LNF

C. Di Giulio, F. Cardelli, S. Pioli +27

TEX facility if commissioned for high power testing to characterize accelerating structures and validate them for the operation on future particle accelerators for medical, industr…

physics.acc-ph2023★ 1 cited

EuPRAXIA@SPARC_LAB Status Update

Fabio Villa

EuPRAXIA@SPARC_LAB is a new multi-disciplinary user-facility that is currently under construction at the Laboratori Nazionali di Frascati of the INFN in the framework of the EuPRAX…

physics.acc-ph2018★ 3 cited

Conceptual design of electron beam diagnostics for high brightness plasma accelerator

A. Cianchi, D. Alesini, M. P. Anania +17

A design study of the diagnostics of a high brightness linac, based on X-band structures, and a plasma accelerator stage, has been delivered in the framework of the EuPRAXIA@SPARC_…

astro-ph.HE2017

The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part III: Cosmic Rays

IceCube Collaboration, M. G. Aartsen, M. Ackermann +312

Papers on cosmic-ray measurements submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration

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★ 179 cited

Extending the search for muon neutrinos coincident with gamma-ray bursts in IceCube data

M. G. Aartsen, M. Ackermann, J. Adams +305

We present an all-sky search for muon neutrinos produced during the prompt -ray emission of 1172 gamma-ray bursts (GRBs) with the IceCube Neutrino Observatory. The detection of…

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.HE2017★ 37 cited

Neutrinos and Cosmic Rays Observed by IceCube

IceCube Collaboration, M. G. Aartsen, M. Ackermann +303

The core mission of the IceCube Neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures…

astro-ph.HE2016★ 198 cited

The IceCube Realtime Alert System

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

Following the detection of high-energy astrophysical neutrinos in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly…

astro-ph.HE2016★ 195 cited

Search for annihilating dark matter in the Sun with 3 years of IceCube data

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

We present results from an analysis looking for dark matter annihilation in the Sun with the IceCube neutrino telescope. Gravitationally trapped dark matter in the Sun's core can a…

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…

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…

astro-ph.HE2016★ 323 cited

All-sky search for time-integrated neutrino emission from astrophysical sources with 7 years of IceCube data

IceCube Collaboration, M. G. Aartsen, K. Abraham +306

Since the recent detection of an astrophysical flux of high energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux come…

astro-ph.HE2016★ 39 cited

First search for dark matter annihilations in the Earth with the IceCube Detector

IceCube Collaboration, M. G. Aartsen, K. Abraham +312

We present the results of the first IceCube search for dark matter annihilation in the center of the Earth. Weakly Interacting Massive Particles (WIMPs), candidates for dark matter…

astro-ph.HE2016★ 514 cited

Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data

IceCube Collaboration, M. G. Aartsen, K. Abraham +309

The IceCube Collaboration has previously discovered a high-energy astrophysical neutrino flux using neutrino events with interaction vertices contained within the instrumented volu…

astro-ph.HE2016

Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube

IceCube Collaboration, M. G. Aartsen, K. Abraham +309

We report constraints on the sources of ultra-high-energy cosmic ray (UHECR) above GeV, based on an analysis of seven years of IceCube data. This analysis efficiently sele…

astro-ph.HE2016★ 7 cited

Search for Sources of High Energy Neutrons with Four Years of Data from the IceTop Detector

IceCube Collaboration, M. G. Aartsen, K. Abraham +308

IceTop is an air shower array located on the Antarctic ice sheet at the geographic South Pole. IceTop can detect an astrophysical flux of neutrons from Galactic sources as an exces…

hep-ex2016★ 74 cited

PINGU: A Vision for Neutrino and Particle Physics at the South Pole

Gen2 Collaboration

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on t…

astro-ph.HE2016★ 31 cited

Lowering IceCube's Energy Threshold for Point Source Searches in the Southern Sky

IceCube Collaboration, M. G. Aartsen, K. Abraham +317

Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cosmic-ray accelerator. While IceCube has recently discovered a diffuse flux of ast…

astro-ph.HE2016★ 62 cited

All-flavour Search for Neutrinos from Dark Matter Annihilations in the Milky Way with IceCube/DeepCore

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

We present the first IceCube search for a signal of dark matter annihilations in the Milky Way using all-flavour neutrino-induced particle cascades. The analysis focuses on the Dee…

physics.acc-ph2016

Linear Accelerator Test Facility at LNF Conceptual Design Report

Paolo Valente, Maurizio Belli, Bruno Bolli +25

Test beam and irradiation facilities are the key enabling infrastructures for research in high energy physics (HEP) and astro-particles. In the last 11 years the Beam-Test Facility…

astro-ph.HE2016★ 118 cited

Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector

IceCube Collaboration, M. G. Aartsen, K. Abraham +314

The IceCube Neutrino Observatory has accumulated a total of 318 billion cosmic-ray induced muon events between May 2009 and May 2015. This data set was used for a detailed analysis…

astro-ph.HE2016★ 151 cited

An All-Sky Search for Three Flavors of Neutrinos from Gamma-Ray Bursts with the IceCube Neutrino Observatory

IceCube Collaboration, M. G. Aartsen, K. Abraham +314

We present the results and methodology of a search for neutrinos produced in the decay of charged pions created in interactions between protons and gamma-rays during the prompt emi…