0000000001250411

AUTHOR

I. Rees

showing 8 related works from this author

Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data

2015

Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of $60\,\mathrm{TeV}$ to the $\mathrm{PeV}$-scale. The origin of those events, being a key to understanding the origin of cosmic rays, is still an unsolved question. So far, analyses have not succeeded to resolve the diffuse signal into point-like sources. Searches including a maximum-likelihood-ratio test, based on the reconstructed directions and energies of the detected down- and up-going neutrino candidates, were also performed on IceCube data leading to the exclusion of bright point sources. In this paper, we present two methods to search for faint neutrino point sources in three years o…

J.2Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScale (descriptive set theory)AstrophysicsIceCubelaw.inventionTelescopelawPoint (geometry)Anisotropyastro-ph.HE2pt-correlationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh Energy Physics::Phenomenology2pt-correlation; Astrophysical neutrinos; Extraterrestrial neutrinos; IceCube; Multipole analysis; Point sourcesAstrophysics::Instrumentation and Methods for AstrophysicsPoint sourcesAstronomyAstronomy and AstrophysicsMultipole analysis3. Good health85-05Astrophysical neutrinosddc:540Extraterrestrial neutrinosHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMultipole expansionGamma-ray burstAstroparticle Physics
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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1~TeV and 1~PeV in 641 days of data taken from 2010--2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far bel…

HIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsParticle physicsAMANDAMesonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESFOS: Physical sciencesCosmic rayAstrophysicsFLUX PREDICTIONS01 natural sciencesIceCube Neutrino ObservatoryIceCubeObservatorySEARCH0103 physical sciencesddc:530Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPERFORMANCEBLAZARSPROMPT LEPTONSGAMMA-RAYPhysics and AstronomyHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsPhysical Review D
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X Chromosome Contribution to the Genetic Architecture of Primary Biliary Cholangitis

2021

Background & aims: Genome-wide association studies in primary biliary cholangitis (PBC) have failed to find X chromosome (chrX) variants associated with the disease. Here, we specifically explore the chrX contribution to PBC, a sexually dimorphic complex autoimmune disease. Methods: We performed a chrX-wide association study, including genotype data from 5 genome-wide association studies (from Italy, United Kingdom, Canada, China, and Japan; 5244 case patients and 11,875 control individuals). Results: Single-marker association analyses found approximately 100 loci displaying P < 5 × 10-4, with the most significant being a signal within the OTUD5 gene (rs3027490; P = 4.80 × 10-6; odds…

Canadian-US PBC Consortium0301 basic medicineMaleLinkage disequilibriumGenome-wide association studyDiseasePBCSettore MED/03 - GENETICA MEDICALinkage Disequilibrium0302 clinical medicineUK-PBC ConsortiumGenotypeMitochondrial Precursor Protein Import Complex ProteinsItalian PBC Genetics Study GroupOdds RatioX-Wide Association StudyJapan PBC-GWAS ConsortiumX chromosomeGeneticsLiver Cirrhosis BiliaryGastroenterologyForkhead Transcription FactorsDNA-Binding ProteinsShal Potassium Channels030211 gastroenterology & hepatologyFemaleAdultMonosaccharide Transport ProteinsSuperenhancerLocus (genetics)Single-nucleotide polymorphismBiologyProtein Serine-Threonine KinasesPolymorphism Single NucleotideArticleWhite People03 medical and health sciencesAsian PeopleProto-Oncogene ProteinsEndopeptidasesHumansCell LineageGenetic Predisposition to DiseaseMeta-analysiGenetic associationChromosomes Human XGastroenterology & HepatologyHepatology1103 Clinical SciencesMeta-analysis030104 developmental biologyGenetic Loci1114 Paediatrics and Reproductive MedicineMeta-analysis; Superenhancer; X-Wide Association Study1109 NeurosciencesCarrier ProteinsGenome-Wide Association Study
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Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data

2014

We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a region of denser instrumentation, enables the detection and reconstruction of atmospheric muon neutrinos between 10 GeV and 100 GeV, where a strong disappearance signal is expected. The detector volume surrounding DeepCore is used as a veto region to suppress the atmospheric muon background. Neutrino events are selected where the detected Cherenkov photons of the secondary particles minimally scatter, and the neutrino energy and arrival direction are reconstructed. Both variables are used to obtain the neutrino oscilla…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsTELESCOPEPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)TRACK RECONSTRUCTIONMuon neutrinoddc:530Neutrino oscillationPhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Solar neutrino problemPERFORMANCENeutrino detectorPhysics and AstronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoNeutrino astronomySYSTEM
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Corrigendum to ‘An international genome-wide meta-analysis of primary biliary cholangitis: Novel risk loci and candidate drugs’ [J Hepatol 2021;75(3)…

2022

It has come to our attention that the name of one of the authors in our manuscript was incorrectly spelled ‘Jinyoung Byan’; the correct spelling is ‘Jinyoung Byun’ as in the author list above. In addition, the excel files of the supplementary tables were not included during the online publication of our article. These have now been made available online. We apologize for any inconvenience caused.

PBC
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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

2014

Made available in DSpace on 2022-04-29T07:21:49Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-11-17 We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of …

MECHANISMPhysics and Astronomy (miscellaneous)AstrophysicsFOLLOW-UP OBSERVATIONSASTROPHYSICAL SOURCESIceCubeneutrinoDetection of gravitational waveGravitational waves neutrinoObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCLIGO Scientific CollaborationQBPhysicsGAMMA-RAY BURSTS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYNuclear and High Energy Physics; Physics and Astronomy (miscellaneous)NEUTRINOSNeutrino detectorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoSENSITIVITYGIANT FLARENuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]95.85.RyMUON NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATIONGravitational wavesGeneral Relativity and Quantum CosmologyINSTABILITIESSettore FIS/05 - Astronomia e AstrofisicaCORE-COLLAPSE SUPERNOVAE[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530SDG 7 - Affordable and Clean EnergyCORE-COLLAPSEDETECTOR/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyGravitational wave95.85.SzMAGNETIZED NEUTRON-STARS[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyTRANSIENTS95.85.Sz; 95.85.RyRELATIVISTIC STARSLIGOPhysics and Astronomy[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma-ray burstEMISSIONEnergy (signal processing)
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Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

2015

A diffuse flux of astrophysical neutrinos above $100\,\mathrm{TeV}$ has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to $35\,\mathrm{TeV}$ and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for shower-like events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the $(f_e:f_{\mu}:f_\tau)_\oplus\approx(1:1:1)_\oplus$ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sou…

FLUXAMANDAParticle physicsPhysics::Instrumentation and DetectorsENERGIESAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysicsACCELERATION01 natural sciencesflavor : ratioHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)PionObservatory0103 physical sciencesddc:550010306 general physicsNeutrino oscillationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsSigmashowersCOSMIC-RAYSatmosphere : backgroundtracksneutrino : flavor : rationeutrino : oscillationfluxobservatoryPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenaneutrino : VHEpi : decay
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