Search results for "Veto techniques"

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Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

2020

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atm…

background [atmosphere]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenapoleFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubecharged currentHigh Energy Physics - Experiment (hep-ex)Neutrinos; Point sources; Veto techniquesSEARCHTRACK RECONSTRUCTION0103 physical sciencessupernovaMuon neutrinoatmosphere [muon]Neutrinos010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsneutrino muonMuon010308 nuclear & particles physicsICEGalactic CenterHigh Energy Physics::PhenomenologyVeto techniquesAstronomyPoint sourcesAstronomy and Astrophysicsflux [neutrino]Galactic planeobservatorySupernovaPhysics and AstronomySkyenergy [neutrino]gamma rayddc:540spectralHigh Energy Physics::ExperimentgalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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