Search results for " Database"

showing 10 items of 684 documents

Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

2015

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15∘. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with …

AstrofísicaPhysics and Astronomy (miscellaneous)Raycosmic radiation anisotropy cosmic radiation propagation cosmic radiation deflectionAstronomymagnetic fieldpAstrophysicsanisotropy [cosmic radiation]01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareAugerPierre//purl.org/becyt/ford/1 [https]ObservatoryJetsQuantum Chromodynamicscosmic radiation: VHEenergy: correlationPatternsMonte Carlo010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic radiation: propagationEnergyCOSMIC cancer databaseAngular distance[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleSearchAstrophysics::Instrumentation and Methods for Astrophysicscosmic radiation anisotropyPierre Auger Observatorycosmic radiation: deflectionRadiación cósmicaAugerSurface Detector ArrayCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaPrincipal axis theorem[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Regular Article - Experimental PhysicsAstrophysics::High Energy Astrophysical PhenomenaPhysics and Astronomy (miscellaneous) Engineering (miscellaneous).FOS: Physical sciencesCosmic ray530cosmic radiation: anisotropyParticle detectorSettore FIS/05 - Astronomia e AstrofisicaVHE [cosmic radiation]statistical analysisSpectrum0103 physical sciencesthrustddc:530Engineering (miscellaneous)AstrophysiqueCiencias ExactasPierre Auger Observatoryair: showerscosmic radiation propagationPhysics and Astronomy (miscellaneous); Engineering (miscellaneous)010308 nuclear & particles physicsturbulence[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstroparticles//purl.org/becyt/ford/1.3 [https]ASTROFÍSICAGalactic Magnetic-fieldcorrelation [energy]DirectionExperimental High Energy Physicscosmic radiation deflectionpropagation [cosmic radiation]direct detectiongalaxyObservatory[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]deflection [cosmic radiation]showers [air]Model
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Dark coupling

2009

30 pages, 10 figures, 3 tables.-- Pre-print archive.

AstrofísicaPhysicsCouplingCosmology and Nongalactic Astrophysics (astro-ph.CO)COSMIC cancer databasemedia_common.quotation_subjectFOS: Physical sciencesPerturbation (astronomy)Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmology of Theories beyond the SMCurvatureCMB cold spotCosmological perturbation theoryUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark energy theoryDark energyNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_commonJournal of Cosmology and Astroparticle Physics
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Calculation of the local density of relic neutrinos

2017

Nonzero neutrino masses are required by the existence of flavour oscillations, with values of the order of at least 50 meV. We consider the gravitational clustering of relic neutrinos within the Milky Way, and used the $N$-one-body simulation technique to compute their density enhancement factor in the neighbourhood of the Earth with respect to the average cosmic density. Compared to previous similar studies, we pushed the simulation down to smaller neutrino masses, and included an improved treatment of the baryonic and dark matter distributions in the Milky Way. Our results are important for future experiments aiming at detecting the cosmic neutrino background, such as the Princeton Tritiu…

AstrofísicaPhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)CosmologiaCOSMIC cancer database010308 nuclear & particles physicsMilky WayHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesCosmic neutrino backgroundBaryon0103 physical sciencesNeutrino010303 astronomy & astrophysicsEvent (particle physics)Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Testing LTB void models without the cosmic microwave background or large scale structure: new constraints from galaxy ages

2012

We present new observational constraints on inhomogenous models based on observables independent of the CMB and large-scale structure. Using Bayesian evidence we find very strong evidence for homogeneous LCDM model, thus disfavouring inhomogeneous models. Our new constraints are based on quantities independent of the growth of perturbations and rely on cosmic clocks based on atomic physics and on the local density of matter.

AstrofísicaVoid (astronomy)Cosmology and Nongalactic Astrophysics (astro-ph.CO)dark energy experimentsCosmic microwave backgroundgalaxy evolutionFOS: Physical sciencesAstrophysicsBayesian evidenceAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences0103 physical sciencesScale structuredark energy theory010303 astronomy & astrophysicsPhysicsCOSMIC cancer databaseCosmologia010308 nuclear & particles physicsAstronomy and AstrophysicsObservableGalaxiesGalaxyGalàxiesCosmologyHomogeneousAstrophysics - Cosmology and Nongalactic Astrophysics
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A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsRayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesantaresAstrophysicsddc:500.2Neutrino fluxesGamma ray burstsPartícules (Física nuclear)law.inventionTelescopeneutrinoRaigs gammalaw14. Life underwaterNeutrinsNeutrinosEngineering (miscellaneous)Cherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon[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 AstrophysicsGamma rayfermi bubbles; antares; neutrinoDetectorCharged particleNeutrino astrophysicsFermi bubbleneutrino telecope13. Climate actionFermi bubblesCol·lisions (Física nuclear):Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAntares neutrino telescopeFermi Gamma-ray Space Telescope
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Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

2018

We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Addi…

Astronomymagnetic fieldAstrophysicsAstrophysics01 natural sciencesAmplitudeastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicscosmic rayastroparticle physics cosmic raysRight ascensionHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HECOSMIC cancer databaseORIGINOBSERVATÓRIOSPhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicAugerastroparticle physics; cosmic rays; Astronomy and Astrophysics; Space and Planetary ScienceobservatorymodulationAmplitudeastroparticle physicsCosmic cancer databaseAstrophysics - High Energy Astrophysical Phenomenalarge scale anysotropysplittingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)cosmic radiation: anisotropycosmic rays0103 physical sciencesHigh Energy Physicscosmic radiation: UHEPierre auger observatoryPierre Auger Observatoryextragalactic origin010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsContext (language use)Astronomy and AstrophysicCosmic rayDipoleSpace and Planetary ScienceExperimental High Energy PhysicsAnisotropyDipoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Right ascensionlarge scale anysotropy extragalactic origindipole
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Measurement of the Cosmic Ray Helium Energy Spectrum from 70 GeV to 80 TeV with the DAMPE Space Mission

2021

The measurement of the energy spectrum of cosmic ray helium nuclei from 70 GeV to 80 TeV using 4.5 years of data recorded by the DArk Matter Particle Explorer (DAMPE) is reported in this work. A hardening of the spectrum is observed at an energy of about 1.3 TeV, similar to previous observations. In addition, a spectral softening at about 34 TeV is revealed for the first time with large statistics and well controlled systematic uncertainties, with an overall significance of $4.3\sigma$. The DAMPE spectral measurements of both cosmic protons and helium nuclei suggest a particle charge dependent softening energy, although with current uncertainties a dependence on the number of nucleons canno…

Astrophysics::High Energy Astrophysical PhenomenaDark matterGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesCosmic raySpace (mathematics)01 natural sciences7. Clean energyCosmic ray heliumHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesEnergy spectrumcosmic rays dark matter spacecrystals010306 general physicsHeliumPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer databasedetectorSettore FIS/01 - Fisica SperimentalecalibrationchemistryParticleAstrophysics - High Energy Astrophysical PhenomenaNucleonperformance
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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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Database Versioning 2.0, a Transparent SQL Approach Used in Quantitative Management and Decision Making

2015

Abstract Managerial decisions are based on accurate information and in today's time raw data is produced even with a stroke of a key. Regardless of the data creating process one needs to know how the information was extracted and which pool of data was used. One important factor is time therefore we need to structure it in layers of data history in such a way that it can be analyzed, (post)process, in order to be able to retrieve valuable information. The simplest way is to use a Database Management System (DBMS), but even with such a management system we face the issue of making it a self-contained database on each version of data added. Our proposed system, a continuation of previous work…

AutocommitSQLPhysical data modelComputer scienceViewData definition languagecomputer.software_genreDatabase designDatabase testingData modelingDecision Making ;DBMSGeneral Environmental Sciencecomputer.programming_languageDatabase modelData administrationSQLDatabasebusiness.industryComponent-oriented databaseDatabase Logical Version ControlAnalyticsGeneral Earth and Planetary SciencesbusinessRaw datacomputerIntelligent databaseProcedia Computer Science
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Preliminary results of the project A.I.D.A. (Auto Immunity: Diagnosis Assisted by computer)

2014

In this paper, are presented the preliminary results of the A.I.D.A. (Auto Immunity: Diagnosis Assisted by computer) project which is developed in the frame of the cross-border cooperation Italy-Tunisia. According to the main objectives of this project, a database of interpreted Indirect ImmunoFluorescence (IIF) images on HEp 2 cells is being collected thanks to the contribution of Italian and Tunisian experts involved in routine diagnosis of autoimmune diseases. Through exchanging images and double reporting; a Gold Standard database, containing around 1000 double reported IIF images with different patterns including negative tests, has been settled. This Gold Standard database has been us…

Autoimmunity ImmunoFluorescence Database Gold Standard CAD Patterns AccuracySettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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