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Kael Hanson

Researcher at University of Wisconsin-Madison

Publications -  486
Citations -  30543

Kael Hanson is an academic researcher from University of Wisconsin-Madison. The author has contributed to research in topics: Neutrino & Neutrino detector. The author has an hindex of 91, co-authored 455 publications receiving 27176 citations. Previous affiliations of Kael Hanson include University of Pennsylvania & Université libre de Bruxelles.

Papers
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Observation of high-energy astrophysical neutrinos in three years of icecube data

M. G. Aartsen, +302 more
TL;DR: Results from an analysis with a third year of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV-PeV range at the level of 10(-8) GeV cm-2 s-1 sr-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ.
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First observation of PeV-energy neutrinos with IceCube

M. G. Aartsen, +287 more
TL;DR: These two neutrino-induced events could be a first indication of an astrophysical neutrinos flux; the moderate significance, however, does not permit a definitive conclusion at this time.
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Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

M. G. Aartsen, +329 more
- 13 Jul 2018 - 
TL;DR: In this article, a high-energy neutrino event detected by IceCube on 22 September 2017 was coincident in direction and time with a gamma-ray flare from the blazar TXS 0506+056.
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Optical properties of deep glacial ice at the South Pole

Markus Ackermann, +116 more
TL;DR: In this article, the authors used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice.
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OBSERVATION and CHARACTERIZATION of A COSMIC MUON NEUTRINO FLUX from the NORTHERN HEMISPHERE USING SIX YEARS of ICECUBE DATA

M. G. Aartsen, +316 more
TL;DR: In this paper, an isotropic, unbroken power-law flux with a normalization at 100 TeV neutrino energy of (0.90 -0.27 +0.30) × 10-18 Gev-1 cm-2 s-1 sr-1 and a hard spectral index of γ = 2.13 ± 0.13.