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H. Wissing

Researcher at University of Maryland, College Park

Publications -  177
Citations -  16537

H. Wissing is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Neutrino & Neutrino detector. The author has an hindex of 65, co-authored 176 publications receiving 15615 citations. Previous affiliations of H. Wissing include RWTH Aachen University.

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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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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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A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with icecube

M. G. Aartsen, +319 more
TL;DR: In this article, the results from six different IceCube searches for astrophysical neutrinos in a maximum-likelihood analysis are combined, and the combined event sample features high-statistics samples of shower-like and track-like events.
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Search for dark matter annihilations in the Sun with the 79-string IceCube detector

M. G. Aartsen, +282 more
TL;DR: A search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope is performed, lowering the energy threshold and extending the search to the austral summer.