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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
Introduction Neutrino observations are a unique probe of the universe’s highest-energy phenomena: Neutrinos are able to escape from dense astrophysical environments that photons cannot and areExpand
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Search for dark matter annihilations in the sun with the 79-string IceCube detector.
We have performed 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. For the first time, theExpand
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First observation of the Greisen-Zatsepin-Kuzmin suppression.
The High Resolution Fly's Eye (HiRes) experiment has observed the Greisen-Zatsepin-Kuzmin suppression (called the GZK cutoff) with a statistical significance of five standard deviations. HiRes'Expand
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First observation of PeV-energy neutrinos with IceCube.
We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the highest neutrinoExpand
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Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU)
TLDR
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill array of the IceCube Neutrino Observatory, improving the sensitivity to several aspects of neutrino oscillation physics at modest cost. Expand
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The design and performance of IceCube DeepCore
The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a surface air showerExpand
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Measurement of South Pole ice transparency with the IceCube LED calibration system
The IceCube Neutrino Observatory, approximately 1 km(3) in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by charged particlesExpand
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Energy Reconstruction Methods in the IceCube Neutrino Telescope
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov lightExpand
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Indications of proton-dominated cosmic-ray composition above 1.6 EeV.
We report studies of ultrahigh-energy cosmic-ray composition via analysis of depth of air shower maximum (X(max)), for air shower events collected by the High-Resolution Fly's Eye (HiRes)Expand
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Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live time in 2007. No excessExpand
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