activity
20162020
most citedThe IceCube Neutrino Observatory: Instrumentation and Online Systems

823 citations · 7k across the 68 of their papers we have counts for

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50 papers · 1 filter

astro-ph.HE2020★ 46 cited

IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog

M. G. Aartsen, M. Ackermann, J. Adams +374

Using the IceCube Neutrino Observatory, we search for high-energy neutrino emission coincident with compact binary mergers observed by the LIGO and Virgo gravitational wave (GW) de…

astro-ph.HE2020★ 42 cited

IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae

M. G. Aartsen, M. Ackermann, J. Adams +361

Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized out…

astro-ph.HE2020★ 69 cited

Combined search for neutrinos from dark matter self-annihilation in the Galactic Centre with ANTARES and IceCube

ANTARES Collaboration, A. Albert, M. André +495

We present the results of the first combined dark matter search targeting the Galactic Centre using the ANTARES and IceCube neutrino telescopes. For dark matter particles with mass…

astro-ph.HE2020★ 46 cited

ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky

ANTARES Collaboration, A. Albert, M. André +498

A search for point-like and extended sources of cosmic neutrinos using data collected by the ANTARES and IceCube neutrino telescopes is presented. The data set consists of all the…

astro-ph.HE2020★ 276 cited

Characteristics of the diffuse astrophysical electron and tau neutrino flux with six years of IceCube high energy cascade data

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

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010 -- 2015. Assuming standard oscillations, the astro…

astro-ph.HE2020★ 38 cited

A search for IceCube events in the direction of ANITA neutrino candidates

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

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate event…

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.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.HE2019

A search for IceCube events in the direction of ANITA neutrino candidates

Alex Pizzuto, Anastasia Barbano, Teresa Montaruli +1

The Antarctic Impulsive Transient Antenna (ANITA) collaboration has reported a total of three neutrino candidates from the experiment's first three flights. One of these was the lo…

astro-ph.HE2019

Low Energy Cosmic Ray Spectrum from 250 TeV to 10 PeV using IceTop

Ramesh Koirala, Thomas K. Gaisser

Using IceTop, the surface component of the IceCube Neutrino Observatory, the all-particle cosmic ray energy spectrum has been determined above a few PeV. The measured energy spectr…

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.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…

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…

astro-ph.HE2018★ 42 cited

Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube

ANTARES, IceCube, LIGO +1589

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-th…

astro-ph.HE2018★ 13 cited

Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector

IceCube Collaboration, M. G. Aartsen, M. Ackermann +326

We report on the observation of a deficit in the cosmic ray flux from the directions of the Moon and Sun with five years of data taken by the IceCube Neutrino Observatory. Between…

astro-ph.HE2018★ 92 cited

Joint constraints on Galactic diffuse neutrino emission from ANTARES and IceCube

A. Albert, M. André, M. Anghinolfi +454

The existence of diffuse Galactic neutrino production is expected from cosmic ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offeri…

astro-ph.HE2018★ 39 cited

Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

M. G. Aartsen, M. Ackermann, J. Adams +331

High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets and n…