Search results for "Cube"

showing 10 items of 160 documents

On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

2006

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN mode…

AMANDAActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIceCubeLuminosityAGNNeutrinosBlazarAstrophysics::Galaxy AstrophysicsAGN; AMANDA; IceCube; Neutrinos; Point sources; Source stackingAstroparticle physicsPhysicsAstrophysics (astro-ph)Point sourcesAstronomyAstronomy and AstrophysicsQuasarSource stackingNeutrino detectorAstronomiaHigh Energy Physics::ExperimentNeutrino
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Measurement of the AtmosphericνeSpectrum with IceCube

2015

We present a measurement of the atmospheric $\nu_e$ spectrum at energies between 0.1 TeV and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric $\nu_e$ originate mainly from the decays of kaons produced in cosmic-ray air showers. This analysis selects 1078 fully contained events in 332 days of livetime, then identifies those consistent with particle showers. A likelihood analysis with improved event selection extends our previous measurement of the conventional $\nu_e$ fluxes to higher energies. The data constrain the conventional $\nu_e$ flux to be $1.3^{+0.4}_{-0.3}$ times a baseline prediction from a Honda's calculation, including the knee of the cosmic-…

AMANDANuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaHadronCASCADES01 natural sciences7. Clean energyPower lawIceCubeNuclear physicsFlux (metallurgy)DESIGNLikelihood analysisDIGITIZATION0103 physical sciencesNEUTRINO FLUX010306 general physicsDETECTORPhysics010308 nuclear & particles physicsICEHigh Energy Physics::PhenomenologySpectrum (functional analysis)DetectorPERFORMANCEENERGY-SPECTRUMEvent selectionPhysics and AstronomyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsSYSTEMPhysical Review D
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The IceCube data acquisition system: Signal capture, digitization, and timestamping

2008

IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital Optical Modules (DOMs), detect, digitize and timestamp the signals from optical Cherenkov-radiation photons. The DOM Main Board (MB) data acquisition subsystem is connected to the central DAQ in the IceCube Laboratory (ICL) by a single twisted copper wire-pair and transmits packetized data on demand. Time calibration is maintained throughout the array by regular transmission to the DOMs of precisely timed analog signals, synchronized to a central GPS-disciplined clock. The design goals and consequent features, func…

AMANDANuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesAstrophysicsNeutrino telescopeSignalHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryNuclear physicsHigh Energy Physics - Experiment (hep-ex)IcecubeData acquisitionSignal digitizationddc:530Nuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationPhysicsbusiness.industryAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAMANDA; Icecube; Neutrino telescope; Signal digitizationTimestampingInstrumentation and Detectors (physics.ins-det)Analog signalTransmission (telecommunications)Systems designTimestampbusinessComputer hardware
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Earth system data cubes unravel global multivariate dynamics

2020

Understanding Earth system dynamics in light of ongoing human intervention and dependency remains a major scientific challenge. The unprecedented availability of data streams describing different facets of the Earth now offers fundamentally new avenues to address this quest. However, several practical hurdles, especially the lack of data interoperability, limit the joint potential of these data streams. Today, many initiatives within and beyond the Earth system sciences are exploring new approaches to overcome these hurdles and meet the growing interdisciplinary need for data-intensive research; using data cubes is one promising avenue. Here, we introduce the concept of Earth system data cu…

Agriculture and Food SciencesDECOMPOSITION0106 biological sciencesFLUXESDependency (UML)lcsh:Dynamic and structural geology010504 meteorology & atmospheric sciencesInterface (Java)Computer scienceDIMENSIONALITY010603 evolutionary biology01 natural sciencesESAData cube03 medical and health scienceslcsh:QE500-639.5TEMPERATURE SENSITIVITYlcsh:Science030304 developmental biology0105 earth and related environmental sciences0303 health sciencesData stream mininglcsh:QE1-996.5SCIENCEFRAMEWORKData sciencePRODUCTSlcsh:GeologyMODELEarth system scienceVariable (computer science)Workflow13. Climate actionGeneral Earth and Planetary Scienceslcsh:QSOIL RESPIRATIONCurse of dimensionality
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Zvaigžņotā Debess: 2017, Pavasaris (235)

2017

Contents: “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: E.Mūkins. Clouds of Venus: Structure and Composition (abridged) ; J.Miezis. 3rd All-union Young Astronomers Gathering (abridged) ; DEVELOPMENTS in SCIENCE: K.Schwartz. New Discoveries in the Milky Way ; DISCOVERIES: I.Eglītis. Small Planets Get Latvian Names ; I.Pundure. Earth-mass World Revealed around Proxima Centauri ; SPACE RESEARCH and EXPLORATION: J.Jaunbergs. Mysteries of Saturn’s Clouds ; A.Slavinskis. Contribution of Estonian Student Satellite Programme ESTCube to Largest Challenges for Humanity ; R.Misa. Impossible Engine that Is likely Possible ; I.Pundure. ESO VLT to Search for Planets in Alpha Centauri System ; EARTH and COSMOS: J.…

Akadēmiķim Oļģertam Dumbrājam – Artura Balklava balva 2017Kosmologs un matemātiķis abats Žoržs LemetrsStarptautiskā matemātikas olimpiāde 2015 – uzdevumu atrisinājumiErnestam Ābelem – 110Pasaules laiks UTC 31.XII 2016. liekā sekunde un LU AI atompulkstenisAsteroīdi – Saule EglitisZemes masas citplanēta Proxima bDzinējs EmDriveIgaunijas Studentu satelītu programma ESTCubeZemes vulkānismsLU Astronomiskais tornis – trešā desmitgadePiena Ceļa galaktika – struktūraSeminārs “Ērglis 2016” MazsalacāESO VLT – planētas Centaura Alfas sistēmāMārīte Eglīte (1951-2016)Vidējās masas melnā cauruma kandidātsTiho Brahe Vēnas salāDebess spīdekļi – 2017.gada pavasarisAgrim J. Kalnājam – 80Nozīmīgākie sasniegumi Latvijas zinātnē 2016:NATURAL SCIENCES::Physics::Astronomy and astrophysics [Research Subject Categories]Saturns – atmosfēraĶīnas nesējraķete CZ-5Mārim Ābelem – 80Zvaigžņotais visums grafikas mākslāIzstāde LU Bibiliotēkā – ar Latviju saistīti asteroīdu nosaukumi
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Risque phytosanitaire (ARP) portant sur Fusarium oxysporum f. sp. cubense (agent pathogène responsable de la maladie de Panama) pour les départements…

2018

Risque phytosanitaire (ARP) portant sur [i]Fusarium oxysporum[/i] f. sp.[u] cubense[/u] (agent pathogène responsable de la maladie de Panama) pour les départements d'Outre-mer

Analyse de risque phytosanitaire[SDV.SA]Life Sciences [q-bio]/Agricultural sciences[SDV.SA] Life Sciences [q-bio]/Agricultural sciencesoutre mer françaisétat de l'artrisque économiqueregulationweed control methodsrace tropicale 4champignon phytopathogèneexpertise scientifiquephytopathogenic fungusbananedétection[SDV.BV.PEP]Life Sciences [q-bio]/Vegetal Biology/Phytopathology and phytopharmacyFoc TR4méthode de luttemaladie de PanamaFusarium oxysporum f. sp. cubenseréglementationpathologie végétale[SDV.BV.PEP] Life Sciences [q-bio]/Vegetal Biology/Phytopathology and phytopharmacyéconomie des filières
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The IceCube prototype string in Amanda

2006

The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole Station. Each OM contains a photomultiplier tube (PMT) that detects photons of Cherenkov light generated in the ice by muons and electrons. IceCube is a cubic-kilometer-sized expansion of Amanda currently being built at the South Pole. In IceCube the PMT signals are digitized already in the optical modules and transmitted to the surface. A prototype string of 41 OMs equipped with this new all-digital technology was deployed in the Amanda array in the year 2000. In this paper we describe the technology and demonst…

Antarctic Muon And Neutrino Detector ArrayAstroparticle physicsPhysicsNuclear and High Energy PhysicsPhotomultiplierPhotonMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Neutrino telescopeAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysicsNeutrino telescopeAmandaIceCubeData acquisitionSignal digitizationAmanda; IceCube; Neutrino telescope; Signal digitizationInstrumentationCherenkov radiation
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Muon track reconstruction and data selection techniques in AMANDA

2004

The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500m and 2000m. The primary goal of this detector is to discover astrophysical sources of high energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of r…

Antarctic Muon And Neutrino Detector ArrayPhysicsAMANDANuclear and High Energy PhysicsParticle physicsAMANDA; Neutrino astrophysics; Neutrino telescope; Track reconstructionMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)DetectorFOS: Physical sciencesAstrophysicsNeutrino telescopeTrack reconstructionNeutrino astrophysicsIceCube Neutrino ObservatoryNeutrino detectorHigh Energy Physics::ExperimentMuon neutrinoNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationLeptonNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Existence of doubling measures via generalised nested cubes

2012

Working on doubling metric spaces, we construct generalised dyadic cubes adapting ultrametric structure. If the space is complete, then the existence of such cubes and the mass distribution principle lead into a simple proof for the existence of doubling measures. As an application, we show that for each $\epsilon>0$ there is a doubling measure having full measure on a set of packing dimension at most $\epsilon$.

Applied MathematicsGeneral MathematicsDyadic cubesStructure (category theory)Space (mathematics)Measure (mathematics)CombinatoricsMetric spacePacking dimension28C15 (Primary) 54E50 (Secondary)Mathematics - Classical Analysis and ODEsSimple (abstract algebra)Classical Analysis and ODEs (math.CA)FOS: MathematicsUltrametric spaceMathematicsProceedings of the American Mathematical Society
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First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope

2013

A search for neutrino-induced muons in correlation with a selection of 40 gamma-ray bursts that occurred in 2007 has been performed with the ANTARES neutrino telescope. During that period, the detector consisted of 5 detection lines. The ANTARES neutrino telescope is sensitive to TeV-PeV neutrinos that are predicted from gamma-ray bursts. No events were found in correlation with the prompt photon emission of the gamma-ray bursts and upper limits have been placed on the flux and fluence of neutrinos for different models.

AstrofísicaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrino experiments; neutrino astronomy; gamma ray bursts theoryPOINT SOURCESPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFluxFOS: Physical sciencesAstrophysics01 natural sciencesICECUBEneutrino astronomyneutrino experiments0103 physical sciencesgamma ray bursts theory010303 astronomy & astrophysicsNeutrino experimentsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonGamma ray bursts theory010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygamma ray bursts theory; neutrino astronomy; neutrino experimentsAstronomy and Astrophysicsgamma ray burstsCATALOGRedshiftNeutrino detectorNeutrino astronomyFISICA APLICADAneutrino experimentHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstSYSTEM
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