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IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica
Gen2 Collaboration, M. G. Aartsen, M. Ackermann +325
The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the "first light" in the nascent field of neutrino astronomy. The observ…
Search for Prompt Neutrino Emission from Gamma-Ray Bursts with IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +300
We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible w…
Measuring a Cherenkov ring in the radio emission from air showers at 110-190 MHz with LOFAR
A. Nelles, P. Schellart, S. Buitink +66
Measuring radio emission from air showers offers a novel way to determine properties of the primary cosmic rays such as their mass and energy. Theory predicts that relativistic tim…
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…
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…
Development of a General Analysis and Unfolding Scheme and its Application to Measure the Energy Spectrum of Atmospheric Neutrinos with IceCube
M. G. Aartsen, M. Ackermann, J. Adams +301
We present the development and application of a generic analysis scheme for the measurement of neutrino spectra with the IceCube detector. This scheme is based on regularized unfol…
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…
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…
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…
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…
Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
IceCube Collaboration, M. G. Aartsen, M. Ackermann +299
Dark matter which is bound in the Galactic halo might self-annihilate and produce a flux of stable final state particles, e.g. high energy neutrinos. These neutrinos can be detecte…
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
Pierre Auger Collaboration, Gabriele Curci
The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the mon…
Search for non-relativistic Magnetic Monopoles with IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +288
The IceCube Neutrino Observatory is a large Cherenkov detector instrumenting of Antarctic ice. The detector can be used to search for signatures of particle phys…
Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU)
PINGU Collaboration
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill array of the IceCube Neutrino Observatory. Leveraging technology proven with IceCube, PINGU w…