0000000001127488

AUTHOR

B. Smith

showing 20 related works from this author

Search for short baseline nu(e) disappearance with the T2K near detector

2015

8 pages.- 6 figures

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoAstronomy & AstrophysicsNeutrino beam7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillation0206 Quantum PhysicsNeutrino fluxPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsDetectorT2K experimentNuclear & Particles Physics0201 Astronomical And Space SciencesPhysical Sciences
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T2K neutrino flux prediction

2013

The Tokai-to-Kamioka (T2K) experiment studies neutrino oscillations using an off-axismuon neutrino beam with a peak energy of about 0.6 GeV that originates at the Japan Proton Accelerator Research Complex accelerator facility. Interactions of the neutrinos are observed at near detectors placed at 280 m from the production target and at the far detector-Super-Kamiokande-located 295 km away. The flux prediction is an essential part of the successful prediction of neutrino interaction rates at the T2K detectors and is an important input to T2K neutrino oscillation and cross section measurements. A FLUKA and GEANT3-based simulation models the physical processes involved in the neutrino producti…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaddc:500.2Antiprotons01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsPions0103 physical sciencesMomentum rangeMuon neutrino010306 general physicsNeutrino oscillationNuclear ExperimentQCPhysicsGev-c010308 nuclear & particles physicsParticle-productionHigh Energy Physics::PhenomenologyT2K experimentFísicaDetectorMonitorSolar neutrino problemNucleiNeutrino detector13. Climate actionMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoProtonsAbsorption cross-sectionsParticle Physics - Experiment
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The liquid-argon scintillation pulseshape in DEAP-3600

2020

AbstractDEAP-3600 is a liquid-argon scintillation detector looking for dark matter. Scintillation events in the liquid argon (LAr) are registered by 255 photomultiplier tubes (PMTs), and pulseshape discrimination (PSD) is used to suppress electromagnetic background events. The excellent PSD performance of LAr makes it a viable target for dark matter searches, and the LAr scintillation pulseshape discussed here is the basis of PSD. The observed pulseshape is a combination of LAr scintillation physics with detector effects. We present a model for the pulseshape of electromagnetic background events in the energy region of interest for dark matter searches. The model is composed of (a) LAr scin…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterFOS: Physical scienceslcsh:AstrophysicsScintillatorWavelength shifter01 natural sciencesParticle detectorDEAPOptics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)PhysicsScintillation010308 nuclear & particles physicsbusiness.industryInstrumentation and Detectors (physics.ins-det)Scintillation counterlcsh:QC770-798businessEuropean Physical Journal C: Particles and Fields
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Measurement of the $\nu_{\mu}$ charged current quasi-elastic cross-section on carbon with the T2K on-axis neutrino beam

2015

17 pages.- 21 figures

Particle physicsNuclear and High Energy Physicschemistry.chemical_elementPion productionAstronomy & AstrophysicsMASSNeutrino beamPION-PRODUCTION7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsScatteringCross section (physics)0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron010306 general physicsNeutrino oscillationNuclear Experiment0206 Quantum PhysicsCharged currentPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsScatteringPhysicsDetectorNuclear & Particles PhysicsMODEL0201 Astronomical And Space ScienceschemistryPhysical SciencesHigh Energy Physics::ExperimentNeutrinoCarbonNuclear targets
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The Stockholm–Mainz ion trap project

1993

A new ion trap facility is described which is dedicated to studies of highly charged ions in a Penning trap. Such a trap will be connected to sources of highly charged ions, in particular the electron beam ion source CRYSIS, at the Manne Siegbahn Institute for Physics. The use of highly charged ions in a Penning trap increases the cyclotron frequency with a factor proportional to the charge which leads to a higher resolution. Also, the possibility to vary the charge state makes it possible to search for and identify different systematic effects. Thus, a substantial increase in accuracy can be expected. In addition, the combination of high charge state ions and a Penning trap allows new appl…

Trap (computing)PhysicsIon trapGeonium atomAtomic physicsCondensed Matter PhysicsIon gunPenning trapMathematical PhysicsAtomic and Molecular Physics and OpticsIon sourceElectron ionizationIonPhysica Scripta
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Measurement of the inclusive $\nu_{\mu}$ charged current cross section on iron and hydrocarbon in the T2K on-axis neutrino beam

2014

We report a measurement of the $\nu_\mu$ inclusive charged current cross sections on iron and hydrocarbon in the T2K on-axis neutrino beam. The measured inclusive charged current cross sections on iron and hydrocarbon averaged over the T2K on-axis flux with a mean neutrino energy of 1.51 GeV are $(1.444\pm0.002(stat.)_{-0.157}^{+0.189}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, and $(1.379\pm0.009(stat.)_{-0.147}^{+0.178}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, respectively, and their cross section ratio is $1.047\pm0.007(stat.)\pm0.035(syst.)$. These results agree well with the predictions of the neutrino interaction model, and thus we checked the correct treatme…

Particle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstronomy & Astrophysics7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationNuclear ExperimentDETECTORCharged currentMathematical Physicschemistry.chemical_classificationPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsT2K experimentFísicaHydrocarbonchemistryPhysical SciencesHigh Energy Physics::ExperimentNuclear and High Energy Physics; Mathematical Physics; Physics and Astronomy (all)NeutrinoNucleon
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Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

2014

The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3$\sigma$ when compared to 4.92 $\pm$ 0.55 expected background events. In the PMNS mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles $\theta_{12}$, $\theta_{23}$, $\theta_{13}$, a mass difference $\Delta m^2_{32}$ and a CP violating phase $\delta_{\mathrm{CP}}$. In this neutrino oscillation scenario, assuming $…

General PhysicsParticle physicsSolar neutrinoPhysics MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomy7. Clean energy09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tau neutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillation01 Mathematical SciencesPhysicsScience & Technology02 Physical Scienceshep-exPhysicsHigh Energy Physics::PhenomenologyT2K experimentFísicaSolar neutrino problemNeutrino detectorT2K CollaborationPhysical SciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Understanding the uncertainty in global forest carbon turnover

2020

Abstract. The length of time that carbon remains in forest biomass is one of the largest uncertainties in the global carbon cycle, with both recent historical baselines and future responses to environmental change poorly constrained by available observations. In the absence of large-scale observations, models used for global assessments tend to fall back on simplified assumptions of the turnover rates of biomass and soil carbon pools. In this study, the biomass carbon turnover times calculated by an ensemble of contemporary terrestrial biosphere models (TBMs) are analysed to assess their current capability to accurately estimate biomass carbon turnover times in forests and how these times a…

0106 biological sciences010504 meteorology & atmospheric sciencesEnvironmental changelcsh:Life01 natural sciencesCarbon cyclelcsh:QH540-549.5ddc:550Baseline (configuration management)Ecology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processes[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereBiomass (ecology)lcsh:QE1-996.5BiosphereSoil carbon15. Life on landPlant functional typelcsh:GeologyEarth scienceslcsh:QH501-531[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionTurnoverlcsh:EcologyPhysical geography010606 plant biology & botanyBiogeosciences
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Measurement of theνμcharged-current quasielastic cross section on carbon with the ND280 detector at T2K

2015

We thank the J-PARC staff for superb accelerator performance and the CERN NA61 Collaboration for providing valuable particle production data. We acknowledge the support of MEXT, Japan; NSERC, NRC, and CFI, Canada; CEA and CNRS/IN2P3, France; DFG, Germany; INFN, Italy; National Science Centre (NCN), Poland; RSF, RFBR, and MES, Russia; MINECO and ERDF funds, Spain; SNSF and SER, Switzerland; STFC, UK; and DOE, USA. We also thank CERN for the UA1/NOMAD magnet, DESY for the HERA-B magnet mover system, NII for SINET4, the WestGrid and SciNet consortia in Compute Canada, GridPP, UK. In addition participation of individual researchers and institutions has been further supported by funds from ERC (…

PhysicsNuclear physicsNuclear and High Energy Physics010308 nuclear & particles physics0103 physical sciencesLibrary scienceDESYEarly career010306 general physics7. Clean energy01 natural sciencesNeutrino scatteringPhysical Review D
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First Muon-Neutrino Disappearance Study with an Off-Axis Beam

2012

We report a measurement of muon-neutrino disappearance in the T2K experiment. The 295-km muon-neutrino beam from Tokai to Kamioka is the first implementation of the off-axis technique in a long-baseline neutrino oscillation experiment. With data corresponding to 1.43 × 10(20) protons on target, we observe 31 fully-contained single μ-like ring events in Super-Kamiokande, compared with an expectation of 104 ± 14(syst) events without neutrino oscillations. The best-fit point for two-flavor νμ → ντ oscillations is sin 2(2θ(23)) = 0.98 and |Δm(2)(32)| = 2.65 × 10(−3) eV2. The boundary of the 90% confidence region includes the points (sin2 (2θ(23)), |Δm(2)(32)|) = (1.0, 3.1 × 10(−3) eV2), (0.84, …

Nuclear and High Energy Physics530 PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.27. Clean energy01 natural sciencesNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Muon neutrino010306 general physicsNeutrino oscillationQCPhysics010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyT2K experimentFísicaPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentBeam (structure)
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Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam

2014

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) …

Particle physicsGeneral PhysicsPhysics MultidisciplinaryMODELSGeneral Physics and AstronomyFOS: Physical sciencesMASS01 natural sciences09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGMuon neutrino010306 general physicsNeutrino oscillationDETECTORMixing (physics)01 Mathematical SciencesPhysicsNeutronsScience & Technology02 Physical Sciences010308 nuclear & particles physicsScatteringOscillationhep-exPhysicsFísicaT2K CollaborationPhysical SciencesSYMMETRIESHigh Energy Physics::ExperimentNeutrinoHigh energy physics Mixing Parameter estimation Parameter extractionConfidence limit Energy dependent Neutrino oscillations Off-axis neutrino beam Oscillation parameters Oscillation probabilities Precise measurements Statistical uncertaintyBeam (structure)Energy (signal processing)
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Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays

2014

We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation $\gamma$-rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to $3.01 \times 10^{20}$ protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the $4-30$ MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background …

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and DetectorsC-12FOS: Physical sciencesAstronomy & Astrophysicslaw.inventionHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsSUPER-KAMIOKANDE DETECTORCross section (physics)High Energy Physics - Experiment (hep-ex)lawEXCITATIONABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGO-16Nuclear ExperimentPhysicsCALIBRATIONScience & TechnologyNeutral currenthep-exPhysicsGamma rayT2K experimentFísica3. Good healthPhysical SciencesNeutrinoWEAKFiducial markerBeam (structure)
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Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

2009

Atmospheric parameters, such as pressure (P), temperature (T) and density (ρ ∝ P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ∼ 10% seasonal modulation and ∼ 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and ρ. The former affects the longitudinal development of air showers while the latter influences the Molière radius and hence the lateral distribution of the shower particles. The model is val…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]: 96.50.sdRadiación CósmicaIMPACTAstronomyExtensive air showerFOS: Physical sciencesCosmic rayAstrophysicsExtensive air showers; UHECR; Atmosphere; Weather01 natural sciencesCOSMIC-RAY CASCADESAugerAtmosphereENERGYObservatory0103 physical sciencesExtensive air showersRECONSTRUCTION96.50.sf010303 astronomy & astrophysicsMolière radiusWeatherInstrumentation and Methods for Astrophysics (astro-ph.IM)96.50.sbPierre Auger ObservatoryPhysics010308 nuclear & particles physicsAtmosphereUHECRDetectorFísicaAstronomy and AstrophysicsPresión AtmosféricaPROFILES[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Longitudinal developmentATMOSFERA (ESTUDO)13. Climate actionExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGClimaAstrophysics - Instrumentation and Methods for Astrophysics
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Measurement of the Inclusive NuMu Charged Current Cross Section on Carbon in the Near Detector of the T2K Experiment

2013

T2K has performed the first measurement of nu(mu) inclusive charged current interactions on carbon at neutrino energies of similar to 1 GeV where the measurement is reported as a flux-averaged double differential cross section in muon momentum and angle. The flux is predicted by the beam Monte Carlo and external data, including the results from the NA61/SHINE experiment. The data used for this measurement were taken in 2010 and 2011, with a total of 10.8 x 10(19) protons-on-target. The analysis is performed on 4485 inclusive charged current interaction candidates selected in the most upstream fine-grained scintillator detector of the near detector. The flux-averaged total cross section is (…

Nuclear and High Energy PhysicsHigher educationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino reactionsLibrary scienceFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Early career010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsbusiness.industry4. EducationNuclear TargetsT2K experimentFísicaRussian federationChristian ministryAngular dependenceHigh Energy Physics::Experimentbusiness
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Regional climate model simulations for Europe at 6 k and 0.2 k yr BP: sensitivity to changes in anthropogenic deforestation

2013

Abstract. This study aims to evaluate the direct effects of anthropogenic deforestation on simulated climate at two contrasting periods in the Holocene, ~6 k BP and ~0.2 k BP in Europe. We apply RCA3, a regional climate model with 50 km spatial resolution, for both time periods, considering three alternative descriptions of the past vegetation: (i) potential natural vegetation (V) simulated by the dynamic vegetation model LPJ-GUESS, (ii) potential vegetation with anthropogenic land cover (deforestation) as simulated by the HYDE model (V + H), and (iii) potential vegetation with anthropogenic land cover as simulated by the KK model (V + K). The KK model estimates are closer to a set of polle…

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Measurement of the Inclusive Electron Neutrino Charged Current Cross Section on Carbon with the T2K Near Detector

2014

The T2K off-axis near detector, ND280, is used to make the first differential cross-section measurements of electron neutrino charged current interactions at energies ~1 GeV as a function of electron momentum, electron scattering angle and four-momentum transfer of the interaction. The total flux-averaged $\nu_e$ charged current cross-section on carbon is measured to be $1.11\pm0.09~(stat)\pm0.18~(syst)\times10^{-38} cm^2/nucleon$. The differential and total cross-section measurements agree with the predictions of two leading neutrino interaction generators, NEUT and GENIE. The NEUT prediction is $1.23\times10^{-38} cm^2/nucleon$ and the GENIE prediction is $1.08\times10^{-38} cm^2/nucleon$…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesParticle detectorsElectronCarbon Electron scattering Electrons Neutrons Testbed7. Clean energyHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentCharged currentPhysicsCharged current Differential cross section Electron momentum Electron neutrino Neutrino interactions Off-axis Total cross section Total fluxFísicaGargamelleHigh Energy Physics::ExperimentNeutrinoNucleonElectron neutrinoElectron scatteringPhysical Review Letters
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Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam

2013

The T2K Collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, vertical bar Delta m(32)(2)vertical bar approximate to 2.4 X 10(-3) eV(2). An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy of 0.6 GeV at the Super-Kamiokande (SK) detector 295 km from the beam's origin. Signal and background predictions are constrained by data from near detectors located 280 m from the neutrino production target. We observe 11 electron neutrino candidate events at the SK detector when a background of 3.3 +/- 0.4(syst) events is expected. The background-only hypothesis is rejected with a p value of 0.0…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesFluxddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Momentum rangeMuon neutrino010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsT2K experimentFísicaHigh Energy Physics::ExperimentNeutrinoAbsorption cross-sectionsElectron neutrinoBeam (structure)
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Early outcomes and complications following cardiac surgery in patients testing positive for coronavirus disease 2019: An international cohort study

2021

The outbreak of severe acute respiratory syndromecoronavirus-2, the cause of coronavirus disease 2019 (COVID-19) in December 2019 represented a global emergency accounting for more than 2.5 million deaths worldwide.1 It has had an unprecedented influence on cardiac surgery internationally, resulting in cautious delivery of surgery and restructuring of services.2 Understanding the influence of COVID-19 on patients after cardiac surgery is based on assumptions from other surgical specialties and single-center studies. The COVIDSurg Collaborative conducted a multicenter cohort study, including 1128 patients, across 235 hospitals, from 24 countries demonstrating perioperative COVID-19 infection…

Pulmonary and Respiratory MedicineMale2019-20 coronavirus outbreakmedicine.medical_specialtyCoronavirus disease 2019 (COVID-19)Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2)complication.ArticleNOCohort Studiesoutcomes; complications; following cardiac surgery; coronavirus disease 2019Postoperative ComplicationsCardiovascular Diseases; Cohort Studies; Female; Humans; Male; Middle Aged; SARS-CoV-2; COVID-19; Cardiac Surgical Procedures; Postoperative ComplicationsInternal medicineCardiovascular DiseasemedicineCardiac Surgical ProcedureHumansIn patientCardiac Surgical ProceduresLS7_4business.industrySARS-CoV-2COVID-19Middle AgedCardiac surgeryCardiovascular DiseasesoutcomeSurgeryFemaleCohort StudieCardiology and Cardiovascular Medicinebusinesscardiac surgery[SDV.MHEP]Life Sciences [q-bio]/Human health and pathologyCohort studyHuman
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Machine learning risk prediction of mortality for patients undergoing surgery with perioperative SARS-CoV-2: the COVIDSurg mortality score

2021

The British journal of surgery 108(11), 1274-1292 (2021). doi:10.1093/bjs/znab183

Cuidado perioperatorioAcademicSubjects/MED00910Settore MED/18 - CHIRURGIA GENERALEMedizinpulmonary complicationspreoperative screeningDatasets as TopicSurgical Procedures Operative/mortality030230 surgeryperioperative care ; surgical procedures ; operative mortality ; machine learning ; sars-cov-2Medical and Health SciencesProcediments quirúrgicsCohort StudiesMachine LearningTumours of the digestive tract Radboud Institute for Health Sciences [Radboudumc 14]0302 clinical medicineModelsProcedimientos quirúrgicosMedicine and Health SciencesCOVIDSurg Collaborative Co-authorsMedicine030212 general & internal medicineskin and connective tissue diseasesRapid Research Communication11 Medical and Health SciencesOperative/mortalitySARS-CoV-19COVID-19/mortalityStatisticalCOVID-19/mortality; Cohort Studies; Datasets as Topic; Humans; Machine Learning; Models Statistical; Risk Assessment; SARS-CoV-2; Surgical Procedures Operative/mortalityCOVID-19; Cohort Studies; Datasets as Topic; Humans; Machine Learning; SARS-CoV-2; Surgical Procedures Operative; Models Statistical; Risk AssessmentAprendizaje automáticoOperativeSurgical Procedures OperativeoutcomeOperativo[SDV.IB]Life Sciences [q-bio]/BioengineeringPatient SafetyAcademicSubjects/MED000106.4 SurgeryLife Sciences & BiomedicineHuman61medicine.medical_specialty616.9Coronavirus disease 2019 (COVID-19)Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2)-.Risk AssessmentNOCOVIDSurg CollaborativeVaccine Related03 medical and health sciencesClinical ResearchBiodefenseCures perioperatòriesAprenentatge automàticMortalitatHumansOperatiusLS7_4Surgical ProceduresScience & TechnologyModels Statisticalbusiness.industrySARS-CoV-2SARS-CoV-2 infectionKirurgiPreventionnot indicatedcovid 19fungiEvaluation of treatments and therapeutic interventionsCOVID-19Perioperativecovid 19; pulmonary complications; postoperative mortality risk; SARS-CoV-2 infection; preoperative screening; vaccinationvaccinationmortalityGood Health and Well BeingMortalidadEmergency medicineSurgeryHuman medicineCohort Studiebusinesspostoperative mortality riskPerioperative care
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A Fermi Gamma-Ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-wave Candidates in Advanced LIGO's First Observing R…

2019

We present a search for prompt gamma-ray counterparts to compact binary coalescence gravitational wave (GW) candidates from Advanced LIGO's first observing run (O1). As demonstrated by the multimessenger observations of GW170817/GRB 170817A, electromagnetic and GW observations provide complementary information about the astrophysical source and, in the case of weaker candidates, may strengthen the case for an astrophysical origin. Here we investigate low-significance GW candidates from the O1 compact-binary coalescence searches using the Fermi Gamma-ray Burst Monitor (GBM), leveraging its all-sky and broad energy coverage. Candidates are ranked and compared to background to measure signific…

AstrofísicaGravitacióAstronomyAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysicsAstronomy & Astrophysicsgeneral [gamma-ray burst]01 natural sciencesCoincidenceCoincident0103 physical sciences010306 general physics010303 astronomy & astrophysicsgravitational waveSTFCQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsastro-ph.HEScience & TechnologySolar flareGravitational wavegamma-ray burst: general; gravitational waves; Astronomy and Astrophysics; Space and Planetary ScienceRCUKAstronomy and AstrophysicsAstronomy and AstrophysicLIGOPhysics and Astronomygravitational wavesSpace and Planetary SciencePhysical Sciencesgamma-ray burst: general; gravitational wavesgeneral; gravitational waves; Astronomy and Astrophysics; Space and Planetary Science [gamma-ray burst]False alarmAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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