Search results for "DeepCore"

showing 2 items of 2 documents

Measurement of the Atmospheric ve flux in IceCube

2012

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496 $\pm$ 66(stat.) $\pm$ 88(syst.) are estimated to be cascade events, including both electron neutrino and neutral current events. The rest of the sample includes residual backgrounds due to atmospheric muons and charged current interactions of atmospheric muo…

DEEPCOREParticle physicsAMANDAPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsSEARCH0103 physical sciencesddc:550010306 general physicsNeutrino oscillationDETECTORPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundNeutrino detectorPhysics and Astronomy13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNEUTRINO-INDUCED CASCADESAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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The design and performance of IceCube DeepCore

2011

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 shower array, and a new buried component called DeepCore. DeepCore was designed to lower the IceCube neutrino energy threshold by over an order of magnitude, to energies as low as about 10 GeV. DeepCore is situated primarily 2100 m below the surface of the icecap at the South Pole, at the bottom center of the existing IceCube array, and began taking physics data in May 2010. Its location takes advantage of the exceptionally clear ice at those depths and allows it to use the surrounding IceCube detector a…

Physics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAntarticaGeneratorAstrophysicsNeutrino telescope01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryAntarctica; DeepCore; Detector; IceCube; NeutrinoIceCubeHigh Energy Physics - Experiment (hep-ex)WIMP0103 physical sciencesNeutrino010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsMuon010308 nuclear & particles physicsIceICEAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsDetectorInstrumentation and Detectors (physics.ins-det)GENERATORDeepCoreSupernovaAir showerPhysics and AstronomyNeutrino detector13. Climate actionddc:540AntarcticaHigh Energy Physics::ExperimentNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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