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20102026
most citedThe IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data

380 citations · 3.7k across the 161 of their papers we have counts for

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Showing 2019Show all

17 papers · 1 filter

astro-ph.HE2019★ 12 cited

Searches for neutrinos from cosmic-ray interactions in the Sun using seven years of IceCube data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +358

Cosmic-ray interactions with the solar atmosphere are expected to produce particle showers which in turn produce neutrinos from weak decays of mesons. These solar atmospheric neutr…

astro-ph.HE2019

Neutrino astronomy with the next generation IceCube Neutrino Observatory

M. G. Aartsen, M. Ackermann, J. Adams +399

The past decade has welcomed the emergence of cosmic neutrinos as a new messenger to explore the most extreme environments of the universe. The discovery measurement of cosmic neut…

astro-ph.HE2019★ 10 cited

Constraints on Neutrino Emission from Nearby Galaxies Using the 2MASS Redshift Survey and IceCube

IceCube Collaboration, M. G. Aartsen, M. Ackermann +354

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can tak…

astro-ph.IM2019★ 4 cited

Design and Performance of the first IceAct Demonstrator at the South Pole

M. G. Aartsen, M. Ackermann, J. Adams +393

In this paper we describe the first results of a compact imaging air-Cherenkov telescope, IceAct, operating in coincidence with the IceCube Neutrino Observatory (IceCube) at the ge…

astro-ph.HE2019★ 12 cited

A Search for Neutrino Point-Source Populations in 7 Years of IceCube Data with Neutrino-count Statistics

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

The presence of a population of point sources in a dataset modifies the underlying neutrino-count statistics from the Poisson distribution. This deviation can be exactly quantified…

astro-ph.IM2019

An improved muon track reconstruction for IceCube

Federica Bradascio, Thorsten Glüsenkamp

IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. One of its main objectives is to detect astrophysical neutrinos and identify their sources. High-energ…

astro-ph.HE2019★ 31 cited

A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube

M. G. Aartsen, M. Ackermann, J. Adams +354

We present two searches for IceCube neutrino events coincident with 28 fast radio bursts (FRBs) and one repeating FRB. The first improves upon a previous IceCube analysis -- search…

astro-ph.HE2019★ 15 cited

Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Years of Data from the IceCube Observatory

M. G. Aartsen, M. Ackermann, J. Adams +354

The measurement of diffuse PeV gamma-ray emission from the Galactic plane would provide information about the energy spectrum and propagation of Galactic cosmic rays, and the detec…

astro-ph.HE2019★ 9 cited

The IceCube Neutrino Observatory -- Contributions to the 36th International Cosmic Ray Conference (ICRC2019)

IceCube Collaboration, M. G. Aartsen, M. Ackermann +355

Contributions from the IceCube Collaboration presented at the 36th International Cosmic Ray Conference, 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.HE2019★ 86 cited

Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events

M. G. Aartsen, M. Ackermann, J. Adams +351

Low background searches for astrophysical neutrino sources anywhere in the sky can be performed using cascade events induced by neutrinos of all flavors interacting in IceCube with…

astro-ph.IM2019★ 2 cited

Improving the muon track reconstruction of IceCube and IceCube-Gen2

Federica Bradascio, Thorsten Glüsenkamp

IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect astrophysical neutrinos and identify their sources. High-energy muon neutrinos a…

astro-ph.IM2019★ 7 cited

A unified perspective on modified Poisson likelihoods for limited Monte Carlo data

Thorsten Glüsenkamp

Counting experiments often rely on Monte Carlo simulations for predictions of Poisson expectations. The accompanying uncertainty from the finite Monte Carlo sample size can be inco…

astro-ph.HE2019★ 4 cited

Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +332

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observa…

astro-ph.HE2019★ 59 cited

All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field

HAWC Collaboration, A. U. Abeysekara, R. Alfaro +400

We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the HAWC and IceCube observatories in the Northern and Southern hemis…

hep-ex2019★ 119 cited

Measurement of Atmospheric Tau Neutrino Appearance with IceCube DeepCore

M. G. Aartsen, M. Ackermann, J. Adams +327

We present a measurement of atmospheric tau neutrino appearance from oscillations with three years of data from the DeepCore sub-array of the IceCube Neutrino Observatory. This ana…

astro-ph.HE2019★ 19 cited

Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1

E. Kankare, M. Huber, S. J. Smartt +345

In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. IceCube began releasing alerts for…

astro-ph.HE2019★ 102 cited

Investigation of two Fermi-LAT gamma-ray blazars coincident with high-energy neutrinos detected by IceCube

S. Garrappa, S. Buson, A. Franckowiak +338

After the identification of the gamma-ray blazar TXS 0506+056 as the first compelling IceCube neutrino source candidate, we perform a systematic analysis of all high-energy neutrin…