0000000000384227

AUTHOR

Michael Sutherland

showing 4 related works from this author

The IceCube realtime alert system

2016

Following the detection of high-energy astrophysical neutrinos in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts to the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole detector site and at IceC…

HIGH-ENERGY NEUTRINOSTELESCOPEAstrophysics::High Energy Astrophysical PhenomenaMulti-messenger astronomy; Neutrino astronomy; Neutrino detectors; Transient sources; Astronomy and AstrophysicspoleFOS: Physical sciences01 natural sciencesIceCubelaw.inventionIceCube Neutrino ObservatoryTelescopeSEARCHESCORE-COLLAPSE SUPERNOVAElawObservatory0103 physical sciencesMulti-messenger astronomysiteNeutrino detectors010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsbackgroundEvent (computing)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsPERFORMANCEsensitivityTransient sourcesobservatoryIdentification (information)electromagneticPhysics and AstronomyNeutrino detectorNeutrino astronomyddc:540High Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsFOLLOW-UPAstroparticle Physics
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PINGU: a vision for neutrino and particle physics at the South Pole

2017

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60,000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters $\theta_{\rm 23}$ and $\Delta m^2_{\rm 32}$, including the octan…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmixing [neutrino]atmospheric neutrinos; IceCube Neutrino Observatory; neutrino oscillations; PINGU; Nuclear and High Energy Physicspole7. Clean energy01 natural sciencesPINGUIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - ExperimentObservatoryPhysicssolar [WIMP]precision measurementAstrophysics::Instrumentation and Methods for Astrophysicsoscillation [neutrino]solar [dark matter]atmosphere [neutrino]threshold [energy]mass difference [neutrino]atmospheric neutrinosobservatoryHigh Energy Physics - PhenomenologyUpgradeNeutrino detectorupgradeNeutrinoKM3NETperformanceParticle physicsNuclear and High Energy Physicssupernova [neutrino]particle identification [neutrino/tau]Astrophysics::High Energy Astrophysical PhenomenaSUPERNOVA DETECTIONIceCube Neutrino Observatory0103 physical sciencesOSCILLATIONSmass: low [dark matter]unitarityddc:530010306 general physicsNeutrino oscillationneutrino oscillations010308 nuclear & particles physicsAstronomysensitivityKM3NeTPhysics and Astronomymass [neutrino]beam [neutrino]High Energy Physics::ExperimentgalaxyATMOSPHERIC NEUTRINOSMATTERSYSTEMLeptonmixing angle [neutrino]experimental results
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[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]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Cabbage and fermented vegetables: from death rate heterogeneity in countries to candidates for mitigation strategies of severe COVID-19

2021

International audience; Large differences in COVID-19 death rates exist between countries and between regions of the same country. Some very low death rate countries such as Eastern Asia, Central Europe, or the Balkans have a common feature of eating large quantities of fermented foods. Although biases exist when examining ecological studies, fermented vegetables or cabbage have been associated with low death rates in European countries. SARS-CoV-2 binds to its receptor, the angiotensin-converting enzyme 2 (ACE2). As a result of SARS-CoV-2 binding, ACE2 downregulation enhances the angiotensin II receptor type 1 (AT1 R) axis associated with oxidative stress. This leads to insulin resistance …

ARIA groupAntioxidantMediterranean dietmedicine.medical_treatmentBrassicasulforaphaneMESH: Angiotensin-Converting Enzyme 2ReviewcabbageAntioxidants0302 clinical medicine10183 Swiss Institute of Allergy and Asthma ResearchVegetableskimchiFood sciencekimči0303 health sciencesMESH: NF-E2-Related Factor 23. Good healthAngiotensin-converting enzyme 22723 Immunology and Allergyfermentirana zelenjavaMESH: EcologyKeywords: Angiotensin converting enzyme 2NF-E2-Related Factor 2KEAP1-NRF2 SYSTEMImmunologyReviewsBrassicaNRF203 medical and health sciencesudc:578:635.34:663.15:COVID‐19angiotensin-converting enzyme 2CorrespondenceHumansMESH: SARS-CoV-2LactobacilluINTERMITTENT HYPOXIA2403 ImmunologyScience & TechnologyMESH: HumansAngiotensin II receptor type 1koronavirusMESH: Antioxidantsmedicine.disease030228 respiratory systemchemistryFermentationAllergymedicine.disease_causechemistry.chemical_compoundLINKING GUT MICROBIOTALactobacillalesLactobacillusImmunology and AllergyMESH: COVID-19Angiotensin converting enzyme 2030212 general & internal medicineOXIDATIVE STRESS[SDV.IMM.ALL]Life Sciences [q-bio]/Immunology/AllergologyKeywords: Angiotensin converting enzyme 2; COVID-19; Lactobacillus; cabbage; diet; fermented vegetable; kimchi; sulforaphane.angiotensin-converting enzyme 2; cabbage; COVID-19; diet; fermented vegetable; kimchi; Lactobacillus; sulforaphane2. Zero hungerFOODSEcologyLactobacillalesMortality rate10177 Dermatology ClinicMEDITERRANEAN DIET1107 ImmunologyLife Sciences & Biomedicinefermented vegetable610 Medicine & healthSettore MED/10 - Malattie Dell'Apparato RespiratorioBiologyMESH: FermentationMESH: Gastrointestinal MicrobiomeInsulin resistanceMESH: DietDownregulation and upregulationmedicine030304 developmental biologySARS-CoV-2COVID-19MESH: BrassicaCOVID-19; Lactobacillus; angiotensin-converting enzyme 2; cabbage; diet; fermented vegetable; kimchi; sulforaphane; Angiotensin-Converting Enzyme 2; Antioxidants; COVID-19; Diet; Ecology; Gastrointestinal Microbiome; Humans; Lactobacillales; NF-E2-Related Factor 2; Brassica; Fermentation; SARS-CoV-2; Vegetablesbiology.organism_classificationMESH: VegetablesDYSFUNCTIONDietGastrointestinal MicrobiomeLactobacillusMESH: Lactobacillalesangiotensin-converting enzyme 2 cabbage COVID-19 diet fermented vegetable kimchi Lactobacillus sulforaphanedietOxidative stressSulforaphane
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