activity
20152019
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 897 across the 12 of their papers we have counts for

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Showing astro-ph.HEShow all

23 papers · 1 filter

astro-ph.HE2019

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 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

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

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

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

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…