Search results for "CEC"

showing 10 items of 347 documents

First search for atmospheric and extraterrestrial neutrino-induced cascades with the IceCube detector

2011

We report on the first search for atmospheric and for diffuse astrophysical neutrino-induced showers (cascades) in the IceCube detector using 257 days of data collected in the year 2007-2008 with 22 strings active. A total of 14 events with energies above 16 TeV remained after event selections in the diffuse analysis, with an expected total background contribution of $8.3\pm 3.6$. At 90% confidence we set an upper limit of $E^2\Phi_{90%CL}<3.6\times10^{-7} GeV \cdot cm^{-2} \cdot s^{-1}\cdot sr^{-1} $ on the diffuse flux of neutrinos of all flavors in the energy range between 24 TeV and 6.6 PeV assuming that $\Phi \propto E^{-2}$ and that the flavor composition of the $\nu_e : \nu_\mu : \nu…

HIGH-ENERGY NEUTRINOSSELECTIONNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaHigh-energy neutrinosFOS: Physical sciencesFluxCosmic rayElementary particleAstrophysicsParticle detectorIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SCATTERINGddc:530High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMICEHigh Energy Physics::Phenomenology004Massless particlePhysics and AstronomyNeutrino detectorAMANDA-IIHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenainfo:eu-repo/classification/ddc/004LeptonPhysical Review D
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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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Dipendenza da sostanze ed esperienze sfavorevoli infantili: uno studio empirico condotto con la Childhood Experiences of Care and Abuse Interview (CE…

2015

Backgroud: Numerose ricerche rilevano l’impatto che esperienze sfavorevoli infantili possono avere sulla dipendenza da sostanze. Metodo: 32 tossicodipendenti maschi in trattamento presso comunità e 32 soggetti appartenenti a un gruppo non clinico sono stai intervistati attraverso la Childhood Experience of Care and Abuse. Risultati: La maggior parte dei soggetti del gruppo clinico ha esperito maggiori esperienze (p<0,05) di negligenza, abuso fisico, abuso psicologico e ha ricevuto forme più inadeguate di supervisione e disciplina. Inoltre, i soggetti del gruppo clinico sono stati esposti a un numero più elevato (p=0,01) di esperienze sfavorevoli. Conclusioni: I risultati suggeriscono la pre…

Health (social science)Social PsychologySettore M-PSI/07 - Psicologia DinamicaAbuse Maltreatment Drug Addiction Childhood Experience of Care and Abuse (CECA) Retrospective InterviewDevelopmental and Educational PsychologyAbuso Maltrattamento Tossicodipendenza Childhood Experience of Care and Abuse(CECA) Intervista RetrospettivaMALTRATTAMENTO E ABUSO ALL'INFANZIA
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Measurement of the cosmic ray energy spectrum with IceTop-73

2013

Physical review / D 88(4), 042004 (2013). doi:10.1103/PhysRevD.88.042004

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsFOS: Physical sciencesAstronomyCosmic rayddc:500.2Astrophysics53001 natural sciencesPower lawICECUBEIceCubeIceCube Neutrino ObservatoryAir showerPhysics and AstronomyObservatory0103 physical sciencesEnergy spectrumARRAYddc:530Astrophysics - High Energy Astrophysical Phenomena010306 general physicsphysics
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On the flavor composition of the high-energy neutrinos in IceCube

2016

The IceCube experiment has recently released 3 years of data of the first ever detected high-energy (&gt;30 TeV) neutrinos, which are consistent with an extraterrestrial origin. In this talk, we compute the compatibility of the observed track-to-shower ratio with possible combinations of neutrino flavors with relative proportion (alpha_e:alpha_mu:alpha_tau). Although this observation is naively favored for the canonical (1:1:1) at Earth, once we consider the IceCube expectations for the atmospheric muon and neutrino backgrounds, this flavor combination presents some tension with data. We find that, for an astrophysical neutrino E_nu^{-2} energy spectrum, (1:1:1) at Earth is currently disfav…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsHigh energyParticle physicsMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical scienceshigh-energy neutrinos01 natural sciencesIceCubeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)flavor ratios0103 physical sciencesEnergy spectrumHigh Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaFlavorNuclear and Particle Physics Proceedings
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A next generation Ultra-Fast Flash Observatory (UFFO-100) for IR/optical observations of the rise phase of gamma-ray bursts

2012

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes respond quickly, the number of sub-60 s detections remains small. In mid- to late-2013, the Ultra-Fast Flash Observatory-Pathfinder is to be launched on the Lomonosov spacecraft to investigate early optical GRB emission. This pathfinder mission is necessarily limited in sensitivity and event rate; here we discuss a next generation rapid-response space observatory. We list science topics motivating our instruments, those that require rapid optical-IR GRB response, including: A survey of GRB rise shapes/times, meas…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpacecraftbusiness.industryApertureAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsOrbital mechanicslaw.inventionTelescopeFlash (photography)ObservatorylawbusinessGamma-ray burstAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

2020

In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4$\pi$ steradian field of view and $\sim$99\% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, and to provide valuable insight for other observatories and inform their observing decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these follow up analyses and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analys…

High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysics010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsNeutrino astronomy; High energy astrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesIceCube Neutrino ObservatoryNeutrino astronomySpace and Planetary ScienceObservatory0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High energy astrophysics010303 astronomy & astrophysicsastro-ph.IM0105 earth and related environmental sciencesThe Astrophysical Journal
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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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Jan Karol Chodkiewicz (1686–1712) – szkic biograficzny młodego magnata

2021

Artykuł stanowi próbę zaprezentowania postaci Jana Karola Chodkiewicza z linii supraskiej (1686–1712), syna starosty błudeńskiego i oboźnego wielkiego litewskiego Jerzego Karola Chodkiewicza oraz Marianny Tekli z Naruszewiczów, który do tej pory nie doczekał się żadnego szerszego opracowania naukowego. Podstawę źródłową szkicu biograficznego Chodkiewicza stanowią materiały przechowywane w Archiwum Narodowym w Krakowie, w zespole Archiwum Młynowskie Chodkiewiczów. Różnorodność znajdujących się w nim dokumentów pozwoliła na możliwie jak najdokładniejsze odtworzenie jego życiorysu. Z niego wyłania się postać Jana Karola, który osierocony przez ojca w dzieciństwie zdany był na opiekę swojej mat…

HistorymilitaryBiografijos / BiographiesHistoryVilnius. Vilniaus kraštas (Vilnius region)DK4010-4800media_common.quotation_subjectKrzysztof Stanisław Zawiszajan karol chodkiewicz (1686-1712)HomelandHistory (General)Abiejų Tautų Respublika (ATR; Rzeczpospolita Obojga Narodów; Žečpospolita; Sandrauga; Polish-Lithuanian Commonwealth; Lenkija ir Lietuva; Lenkijos ir Lietuvos Valstybė; Lenkijos-Lietuvos unija)Cecylia Zofia SapieżankaPoliticsLietuva (Lithuania)State (polity)Genealogija. Heraldika / Genealogy. HeraldryGreat Northern War 1700–1721D1-2009History of PolandReligious studiesBejsagołaSupraślQuartermasterPertykówmedia_commonMarianna Tekla NaruszewiczównaeducationBenedykt Paweł SapiehaJonas Karolis Chodkevičius (Jan Karol Chodkiewicz)BiographyUnrestDaugieliszkiWarszawaBłudeńBajorai didikai ir magnatai / Nobles and magnatesmilitary.rankCommonwealthLenkija (Lenkijos karalystė; Rzeczpospolita Polska; Kingdom of Poland; Poland)edukacjaEstatewielka wojna północna 1700–1721Jan Karol Chodkiewicz (1686–1712)WielonaPrzegląd Nauk Historycznych
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Hybrid Anterior Cervical Discectomy
and Fusion and Cervical Disc Arthroplasty: An Analysis of Short-Term Complications, Reoperations, and Readmissions

2022

Hybrid Anterior Cervical Discectomy and Fusion Cervical Disc ArthroplastyOrthopedics and Sports MedicineSurgeryNeurology (clinical)
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