Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

The contribution of the Italian Northern Cross Radiotelescope to the Gamma-Ray Observatory Pulsar Timing Network

1992

The observation of pulsars at gamma-ray energy requires updated pulsar parameters in order to fold the gamma-ray data over time intervals of weeks. The Compton Gamma-Ray Observatory Institute has set up an international agreement including several radiotelescopes and pulsar observers in order to provide a suitable timing support at radio wavelengths. In this paper we describe the system used at the Italian Northern Cross for the pulse timing observations related to the GRO mission.

Radio telescopePhysicsPulsarObservatoryMillisecond pulsarAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomyCosmic rayGamma-ray astronomyAstrophysicsBinary pulsarIl Nuovo Cimento C
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Search for radio pulsations in four anomalous X-ray pulsars and discovery of two new pulsars

2007

We have performed deep searches for radio pulsations from four southern anomalous X-ray pulsars (AXPs) to investigate their physical nature in comparison with the rotation powered pulsars. The data were acquired using the Parkes radio telescope with the 1.4 GHz multibeam receiver. No pulsed emission with periodicity matching the X-ray ephemeris have been found in the observed targets down to a limit of ∼0.1 mJy. A blind search has also been performed on all the 13 beams of the multibeam receiver (the central beam being pointed on the target AXP), leading to the serendipitous discovery of two new radio pulsars and to the further detection of 18 pulsars. Also a search for single dispersed pul…

Radio telescopePhysicsPulsarSpace and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsEphemerisAstrophysics::Galaxy AstrophysicsCosmology
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Search for ultrahigh-energy tau neutrinos with IceCube

2012

The first dedicated search for ultrahigh-energy (UHE) tau neutrinos of astrophysical origin was performed using the IceCube detector in its 22-string configuration with an instrumented volume of roughly 0.25  km3. The search also had sensitivity to UHE electron and muon neutrinos. After application of all selection criteria to approximately 200 live-days of data, we expect a background of 0.60±0.19(stat)+0.56−0.58(syst) events and observe three events, which after inspection, emerge as being compatible with background but are kept in the final sample. Therefore, we set an upper limit on neutrinos of all flavors from UHE astrophysical sources at 90% C.L. of E2νΦ90(νx)<16.3×10−8  GeV cm−2…

SELECTIONAMANDANuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESCosmic rayddc:500.2PROPAGATIONAstrophysicsElectron01 natural sciencesAmanda0103 physical sciencesEARTHddc:530Ultrahigh energy010306 general physicsPropagationSelectionPhysicsRange (particle radiation)Muon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsEarthPhysics and AstronomyInduced CascadesTELESCOPESHigh Energy Physics::ExperimentNeutrinoTelescopes
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A Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-String Detector

2011

The IceCube Neutrino Observatory is a 1 km$^{3}$ detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved sources. A hard energy spectrum of neutrinos from isotropically distributed astrophysical sources could manifest itself as a detectable signal that may be differentiated from the atmospheric neutrino background by spectral measurement. This analysis uses data from the IceCube detector collected in its half completed configuration which operated between April 2008 and May 2009 to search for a diffuse flux of astrophysical muon neutrinos. A to…

SELECTIONAMANDANuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesAmandaIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesddc:530Selection010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuon010308 nuclear & particles physicsICEIceHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsCosmic-RaysSolar neutrino problemCOSMIC-RAYS004MODELPhysics and AstronomyNeutrino detectorTELESCOPESHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomenainfo:eu-repo/classification/ddc/004ModelTelescopesLepton
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"Table 14" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Ratio of cross sections for N/N-1 inclusive jet multiplicities for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

SIG/SIGZ ProductionHigh Energy Physics::PhenomenologyIntegrated Cross SectionAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionCross SectionInclusiveP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentComputer Science::Information Theory
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Ionization and scintillation response of high-pressure xenon gas to alpha particles

2013

High-pressure xenon gas is an attractive detection medium for a variety of applications in fundamental and applied physics. In this paper we study the ionization and scintillation detection properties of xenon gas at 10 bar pressure. For this purpose, we use a source of alpha particles in the NEXT-DEMO time projection chamber, the large scale prototype of the NEXT-100 neutrinoless double beta decay experiment, in three different drift electric field configurations. We measure the ionization electron drift velocity and longitudinal diffusion, and compare our results to expectations based on available electron scattering cross sections on pure xenon. In addition, two types of measurements add…

Scintillation (physics)IonizationMECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsMaterials scienceIonitzacióPhysics::Instrumentation and DetectorsFOS: Physical scienceschemistry.chemical_elementElectronCharge transportNuclear excitation01 natural sciences7. Clean energyHigh Energy Physics - ExperimentTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)Gaseous detectorsXenonComptadors de centelleigIonization and excitation processesIonization0103 physical sciencesPhysics::Atomic and Molecular ClustersNuclear Experiment (nucl-ex)010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Nuclear ExperimentInstrumentationMathematical PhysicsHeliumDetectors de radiacióScintillationTime projection chamber010308 nuclear & particles physicsFísicaMultiplication and electroluminescence in rare gases and liquidsInstrumentation and Detectors (physics.ins-det)Alpha particleDouble-beta decay detectorschemistryNuclear countersScintillation counterExcitació nuclearAtomic physicsAstrophysics - Instrumentation and Methods for Astrophysics
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Contribution of recently measured nuclear data to reactor antineutrino energy spectra predictions

2013

This paper attempts to summarize the actual problematic of reactor antineutrino energy spectra in the frame of fundamental and applied neutrino physics. Nuclear physics is an important ingredient of reactor antineutrino experiments. These experiments are motivated by neutrino oscillations, i.e. the measure of the θ 13 mixing angle. In 2011, after a new computation of the reactor antineutrino energy spectra, based on the conversion of integral data of the beta spectra from 235 U, and 239;241 Pu, a deficit of reactor antineutrinos measured by short baseline experiments was pointed out. This is called the “reactor anomaly”, a new puzzle in the neutrino physics area. Since then, numerous new ex…

Semileptonic decayParticle physicsNuclear and High Energy PhysicsNuclear fission product[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FissionQC1-99901 natural sciences7. Clean energyPhysics::GeophysicsNuclear physics0103 physical sciencesPlutonium-241010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsFission products010308 nuclear & particles physicsPhysicsNuclear dataBeta decay[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Uranium-238Uranium-235High Energy Physics::ExperimentAnomaly (physics)NeutrinoEPJ Web of Conferences
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Different preparation methods of bare and doped carbon nitride (C3N4) employed for selective photocatalytic oxidations

2018

Different preparation methods of bare and doped carbon nitride (C3N4) employed for selective photocatalytic oxidations

Settore CHIM/07 - Fondamenti Chimici Delle TecnologiePreparation methods of bare and doped carbon nitride selective photocatalytic oxidations
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Lithostratigraphy of Sicily

2018

This book offers as comprehensive an overview as possible of the lithostratigraphy of the Italian region of Sicily, taking into account the multiplicity of formational and terminological variability developed over more than a century of studies and publications. It presents stratigraphic terminology, the geological lexicon and the main stratigraphic subdivisions that are not familiar to Sicilian geologists. The new stratigraphic methods and the use of formations as mapping units have prompted the acquisition of new lithostratigraphic data, and a review of the previous units and their comparison with the new collected data, enabling the definition of a number of new lithostratigraphic units.…

Settore GEO/02 - Geologia Stratigrafica E SedimentologicaSedimentology Paleogeography Chronostratigraphy Stratigraphic Methods Plate-tectonic History Micropaleontology Facies Analysis Macro- and Micro-Facies Biostratigraphy Carbonate Deposits Evaporite Deposits
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L'ammortamento alla francese: una questione di trasparenza

2023

Il saggio esamina i numerosi problemi posti dal c.d. metodo di ammortamento alla francese per osservare che buona parte dei problemi dibattuti sorgono dal difficile dialogo tra giuristi e matematici finanziari. Sotto il profilo giuridico rileva, in particolare, che l’ammor- tamento alla francese pone soprattutto problemi di trasparenza delle condizioni contrattuali e di comprensione, da parte del cliente, delle modalità di rimborso del capitale mutuato e dell’entità del debito residuo. The essay examines some problems posed by the so-called French amortization method to observe that most of the debated problems arise from the difficult dialogue between jurists and financial mathematicians. …

Settore IUS/05 - Diritto Dell'Economiaamortization method transparency methods of repayment
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