Search results for "IceTop"

showing 4 items of 4 documents

Cosmic ray composition and energy spectrum from 1–30 PeV using the 40-string configuration of IceTop and IceCube

2012

Astroparticle physics 42, 15 - 32 (2013). doi:10.1016/j.astropartphys.2012.11.003

Knee regionAstrophysicsTracking (particle physics)01 natural sciencesParticle identificationIceCubeTRACKINGWATERCherenkovNeutrino energyNEUTRINO TELESCOPEUltra-high-energy cosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSEADetectorAstrophysics::Instrumentation and Methods for AstrophysicsLIGHTComposition; Cosmic rays; Energy spectrum; IceCube; IceTop; Knee regionddc:540IceTopPARTICLE IDENTIFICATIONAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsIceCube detectorCompositionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2IceCube Neutrino ObservatorySEARCHESAccelerationcosmic raysdE/dx0103 physical sciences010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationTruncated meanMuon energy010308 nuclear & particles physicsAstronomyAstronomy and Astrophysics540Physics and AstronomycompositionEnergy SpectrumTEVEnergy spectrum
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First year performance of the IceCube neutrino telescope

2006

The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence…

Astroparticle physicsPhysicsPhotomultiplierMuonPerformanceDetectorAstrophysics (astro-ph)AstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsIceCube Neutrino ObservatoryAmandaIceCubeDetectionData acquisitionFirst yearAmanda; Detection; First year; IceCube; IceTop; Neutrino; Performance; South poleNeutrinoSouth poleAstronomiaIceTopNeutrinoCherenkov radiation
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All-particle cosmic ray energy spectrum measured with 26 IceTop stations

2012

Astroparticle physics 44, 40 - 58 (2013). doi:10.1016/j.astropartphys.2013.01.016

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2Astrophysics01 natural sciencesIceCubeIceCube Neutrino Observatory0103 physical sciencesCosmic rays010303 astronomy & astrophysicsZenithPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmic rays; Energy spectrum; IceCube; IceTopSpectral indexCOSMIC cancer database010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysics540Air showerKASCADEddc:540IceTopEnergy spectrumNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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IceTop : the surface component of IceCube

2012

IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the mass composition of primary cosmic rays in the energy range from about 100 TeV to 1 EeV by exploiting the correlation between the shower energy measured in IceTop and the energy deposited by muons in the deep ice. In this paper we report on the technical design, construction and installation, the trigger and data acquisition systems as well as the software framework for calibration, reconstruction and simulation. Finally the first experience from commissioning and operating the detector and the performance as an …

FLUXNuclear and High Energy PhysicsAir showerPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAir shower; Cosmic rays; Detector; IceCube; IceTopFOS: Physical sciencesCosmic rayddc:500.27. Clean energy01 natural sciencesIceCube Neutrino ObservatoryIceCubeShowerData acquisitioncosmic raysDIGITIZATION0103 physical sciencesSHOWERSCalibrationddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCosmic raysRemote sensingPhysicsMuondetector010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyDetectorENERGY-SPECTRUMAir showerPhysics and AstronomySIMULATIONIceTopHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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