Search results for "UHE"

showing 10 items of 649 documents

Ultrahigh energy neutrinos in the Mediterranean: Detecting ντ and νμ with a km3 telescope

2007

23 pages, 13 figures.-- PACS nrs.: 95.85.Ry, 95.55.Vj, 13.15.+g.-- ISI Article Identifier: 000245928000025.-- ArXiv pre-print available at: http://arxiv.org/abs/astro-ph/0609241

AstrofísicaHigh energyAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeNeutrino and gamma astronomyAstrophysicslaw.inventionTelescopeAir-showersMediterranean seaUHE-τ neutrinoslawUnderwaterCosmic raysDetectors de radiacióPhysicsCosmologiaNetrino experimentsNetrino detectorsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsNeutrino detectorFluorescence DetectorNeutrinoEnergy (signal processing)
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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

2010

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating…

AstronomyAstrophysicsUltra High Energy Cosmic ray01 natural scienceslaw.inventionObservatorylawAnisotropy010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]UHECRAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKAnisotropíaGALAXIESNEUTRINOSGreisen–Zatsepin–Kuz’minComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEIHIPASS CATALOG[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleusRadiación Cósmicamedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsTelescope0103 physical sciencesCosmic raysCiencias ExactasAstrophysics::Galaxy AstrophysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsAstronomyFísicaAstronomy and AstrophysicsCosmic rayGalaxyCorrelation with astrophysical sourcesCosmic rays; UHECR; Anisotropy; Pierre Auger Observatory; Extra-galactic; GZKSkyExperimental High Energy PhysicsAnisotropyExtra-galactic
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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray …

2018

A new analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby sources. The data consist of 5514 events above 20 EeV with zenith angles up to 80 deg recorded before 2017 April 30. Sky models have been created for two distinct populations of extragalactic gamma-ray emitters: active galactic nuclei from the second catalog of hard Fermi-LAT sources (2FHL) and starburst galaxies from a sample that was examined with Fermi-LAT. Flux-limited samples, which include all types of galaxies from the Swift-BAT and 2MASS …

Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ciencias Físicascosmic radiation: densitygalaxies: starburstAstrophysics01 natural sciences//purl.org/becyt/ford/1 [https]methods: data analysis Supporting material: FITS fileUltra-high-energy cosmic raydata analysis [Methods]Anisotropycosmic radiation: model010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files; Astronomy and Astrophysics; Space and Planetary ScienceAugerobservatorygamma ray: emissiondata analysis Supporting material: FITS file [methods]astroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeData analysisFOS: Physical sciencesStarburstCosmic rayanisotropyAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias FísicasGLASTcosmic raysastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files0103 physical sciencesHigh Energy Physicscosmic radiation: UHEAGNCosmic raysAstrophysics::Galaxy AstrophysicsZenithmethods: data analysis Supporting material: FITS filesPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsIsotropyFísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astronomy and Astrophysicmethods: data analysisGalaxyfluxstarburst [Galaxies]Space and Planetary ScienceExperimental High Energy PhysicsActive galaxiesgalaxyAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statistical
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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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Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube

2020

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can take advantage of these features to establish directional correlations between a neutrino dataset and overdensities in the galaxy distribution in the sky. The results of two correlation searches between a seven-year time-integrated neutrino dataset from the IceCube Neutrino Observatory, and the 2MASS Redshift Survey (2MRS) catalog are presented here. The first analysis searches for neutrinos produced via interactions between diffuse intergalactic Ultra-High Energy Cosmic Rays (UHECRs) and the matter contained within …

Astrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesIceCubeIceCube Neutrino Observatoryneutrino astronomyneutrino experiments0103 physical sciencessiteAstrophysics::Galaxy Astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)densityneutrino astronomy; neutrino detectors; neutrino experiments010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsflux [neutrino]redshiftRedshift surveyGalaxyRedshiftobservatoryNeutrino detectorPhysics and Astronomymultiplet13. Climate actioncorrelationPhysique des particules élémentairesIntergalactic travelHigh Energy Physics::ExperimentgalaxyNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomenaneutrino detectors
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Puhekielen fraasit Augustinuksen Soliloquia-teoksessa

1998

Augustinuksen Soliloquia-teos on dialogimuodossa oleva väittely, joka on hyvä lähde latinan puhekielen fraseologialle. Työn tarkoituksena on esitellä latinankielistä keskustelua helpottavia ilmauksia. Kirkkoisä Augustinus eli myöhäisantiikin aikana, mutta oli silti klassisen latinan edustaja, kuten tässä työssä esiteltävä Soliloquia teoskin osoittaa. Työn pääpaino on kuitenkin latinan puhekielessä. Tästä Augustinuksen ja hänen järkensä välisestä vuoropuhelusta on valikoitu sopivia fraaseja, jotka on suomennettu ja lajiteltu aihepiirinsä mukaan. Varsinaisen käsittelyosan lisäksi fraasit on lueteltu myös suomesta latinaan pain, samoin aihepiirinsä mukaan. Soliloquia-teos oli tarkoitettu kirja…

Augustinus Aureliuspuhekielen fraasit
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The Datafication of Hate: Expectations and Challenges in Automated Hate Speech Monitoring.

2020

Laaksonen, S-M.; Haapoja, J.; Kinnunen, T., Nelimarkka, M. & Pöyhtäri, R. (2020, accepted). . Frontiers in Big Data: Data Mining and Management / Critical Data and Algorithm Studies. doi:10.3389/fdata.2020.00003 Hate speech has been identified as a pressing problem in society and several automated approaches have been designed to detect and prevent it. This paper reports and reflects upon an action research setting consisting of multi-organizational collaboration conducted during Finnish municipal elections in 2017, wherein a technical infrastructure was designed to automatically monitor candidates' social media updates for hate speech. The setting allowed us to engage in a 2-fold investiga…

Big DataComputer sciencehate speechsocial media518 Media and communicationssosiaalinen mediamonitorointi050801 communication & media studiesSocial issues0508 media and communicationspolitiikkadatatiedeArtificial Intelligencealgoritmit050602 political science & public administrationComputer Science (miscellaneous)Social mediaalgorithmic systemvihapuheAction researchObjectivity (science)Original Researchlcsh:T58.5-58.64DataficationSocial phenomenonlcsh:Information technologytekstinlouhinta05 social sciencesCitizen journalism16. Peace & justice113 Computer and information sciencesData science0506 political sciencekoneoppiminenmachine learningNeutralitydata sciencepoliticsInformation Systems
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Coherence between brain activation and speech envelope at word and sentence levels showed age-related differences in low frequency bands

2021

Abstract Speech perception is dynamic and shows changes across development. In parallel, functional differences in brain development over time have been well documented and these differences may interact with changes in speech perception during infancy and childhood. Further, there is evidence that the two hemispheres contribute unequally to speech segmentation at the sentence and phonemic levels. To disentangle those contributions, we studied the cortical tracking of various sized units of speech that are crucial for spoken language processing in children (4.7–9.3 years old, N = 34) and adults (N = 19). We measured participants’ magnetoencephalogram (MEG) responses to syllables, words, and…

Brain activationmagnetoencephalographymedicine.medical_specialtySpeech perceptionLow frequencyAudiologyauditory responsesspeech perception050105 experimental psychologykuulohavainnot03 medical and health sciences0302 clinical medicinekielellinen kehitysmedicine0501 psychology and cognitive sciences[SHS.LANGUE]Humanities and Social Sciences/LinguisticsdevelopmentEnvelope (waves)[SHS.STAT]Humanities and Social Sciences/Methods and statisticsMEGmedicine.diagnostic_test05 social sciencesMagnetoencephalographyCoherence (statistics)[SCCO.LING]Cognitive science/Linguisticsspeech trackingcoherencehavaintopsykologiapuhe (puhuminen)[SCCO.PSYC]Cognitive science/PsychologyPsychology030217 neurology & neurosurgeryWord (computer architecture)Sentence
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Bushilainen maailmanrakenne

2004

Bush George WgeopolitiikkaretoriikkapuheYhdysvallat
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Heroes of Middle-Earth : J. Campbell's monomyth in J. R. R. Tolkien's The Lord of the Rings (1954-1955)

2007

Campbell JosephmonomythheroesTolkien J. R. RThe lord of the ringsmonomyyttisankaritsivuhenkilöt
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