0000000000344268

AUTHOR

Kd De Vries

showing 4 related works from this author

Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube

2017

[EN] The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by ANTARES, within +/- 500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission …

POINT-LIKEGravitational-wave observatoryPhysics and Astronomy (miscellaneous)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyELECTROMAGNETIC COUNTERPARTSastro-ph.HE; astro-ph.HEAstrophysics01 natural sciences7. Clean energylocalizationIceCubeBinary black holeLIGO010303 astronomy & astrophysicsTelescopeGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEFollow-upData-acquisition systemobservatoryNeutrino detectorElectromagnetic counterpartsSIMULATIONBlack-hole mergersLigoGamma-ray burstsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHost galaxiesSimulationGravitational waveBLACK-HOLE MERGERSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesDATA-ACQUISITION SYSTEMGravitational wavesneutrino: productionGeneral Relativity and Quantum CosmologyBinary black holeOnes gravitacionalsLiGO Observatory0103 physical sciencesNeutrinoGW151226ddc:530NeutrinsNeutrinos010306 general physicsPoint-likeANTARESCosmologiaGravitational wavebackgroundgravitational radiationAstronomy530 PhysikLIGONeutron starGravitational Waves Neutrinos Antares IceCube LIGOAntaresPhysics and Astronomyblack hole: binary13. Climate action:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAAstronomiaDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]FOLLOW-UPPhysical Review D. Particles and Fields
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The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays

2011

Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count rates of low energy secondary cosmic ray particles for the self-calibration of the ground detectors of its surface detector array. After correcting for atmospheric effects, modulations of galactic cosmic rays due to solar activity and transient events are observed. Temporal variations related with the activity of the heliosphere can be determined with high accuracy due to the high total count rates. In this study, the available data are presented together with an analysis focused on the observation of Forbush decreases, where a strong correlation with neutron monitor data is found.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010504 meteorology & atmospheric sciencesCherenkov detectorAuger ExperimentAstronomyAstrophysics::High Energy Astrophysical PhenomenaCosmic rayParticle detectorsAstrophysics01 natural sciencesCosmic RayCHERENKOV DETECTORAugerlaw.inventionlaw0103 physical sciencesCherenkov detectors; Large detector systems for particle and astroparticle physics; Particle detectorsBURSTSWATERForbush decreaseUltra-high-energy cosmic ray010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)InstrumentationMathematical Physics0105 earth and related environmental sciencesPhysicsPierre Auger ObservatoryFÍSICA DE PARTÍCULASNeutron monitorLarge detector systems for particle and astroparticle physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov detectorsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Solar activtyExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicFísica nuclearParticle detectorHeliosphereJournal of Instrumentation
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Erratum: The lateral trigger probability function for the ultra-high energy cosmic ray showers detected by the Pierre Auger Observatory (Astroparticl…

2012

The Fig. 7, originally consisting of 4 panels, was truncated in the printed version (the last panel was missing). The complete version is printed again

Astronomy and Astrophysics
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Obser…

2016

This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array. We first consider samples of cascade neutrino events and of high-energy neutrino-induced muon tracks, which provided evidence for a neutrino flux of astrophysical origin, and study their cross-correlation with the ultrahigh-energy cosmic ray (UHECR) samples as a function of angular separation. We also study their possible directional correlations using a likelihood method stacking the neutrino arrival directions and adopting different assumptions on the size…

AstronomyAstrophysicsNeutrino experiments ultra high energy cosmic rays cosmic ray experiments neutrino astronomy.01 natural sciencesASTROPHYSICAL SOURCESultra high energy cosmic raylaw.inventionIceCubeAstronomi astrofysik och kosmologimagnetic [deflection]lawAstronomy Astrophysics and Cosmologycosmic ray experiments; neutrino astronomy; neutrino experiments; ultra high energy cosmic rays; Astronomy and Astrophysics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAngular distanceAstrophysics::Instrumentation and Methods for AstrophysicsVHE [neutrino]GALACTIC MAGNETIC-FIELDcascadeAugerobservatorycosmic radiationCascadestackingcosmic ray experi- mentsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomenaphysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesCosmic rayultra high energy cosmic raysSURFACE DETECTORTelescopeneutrino astronomyneutrino experiments0103 physical sciencesddc:530Angular resolutionHigh Energy PhysicsPierre Auger ObservatorySPECTRUMMuon010308 nuclear & particles physicsAstronomy and Astrophysicsflux [neutrino]ASTROFÍSICAPhysics and Astronomyangular resolutioncorrelationExperimental High Energy Physicsneutrino experimenttracks [muon]cosmic ray experiments
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