Search results for "BEC"

showing 10 items of 947 documents

An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray …

2018

A new analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby sources. The data consist of 5514 events above 20 EeV with zenith angles up to 80 deg recorded before 2017 April 30. Sky models have been created for two distinct populations of extragalactic gamma-ray emitters: active galactic nuclei from the second catalog of hard Fermi-LAT sources (2FHL) and starburst galaxies from a sample that was examined with Fermi-LAT. Flux-limited samples, which include all types of galaxies from the Swift-BAT and 2MASS …

Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ciencias Físicascosmic radiation: densitygalaxies: starburstAstrophysics01 natural sciences//purl.org/becyt/ford/1 [https]methods: data analysis Supporting material: FITS fileUltra-high-energy cosmic raydata analysis [Methods]Anisotropycosmic radiation: model010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files; Astronomy and Astrophysics; Space and Planetary ScienceAugerobservatorygamma ray: emissiondata analysis Supporting material: FITS file [methods]astroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeData analysisFOS: Physical sciencesStarburstCosmic rayanisotropyAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias FísicasGLASTcosmic raysastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files0103 physical sciencesHigh Energy Physicscosmic radiation: UHEAGNCosmic raysAstrophysics::Galaxy AstrophysicsZenithmethods: data analysis Supporting material: FITS filesPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsIsotropyFísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astronomy and Astrophysicmethods: data analysisGalaxyfluxstarburst [Galaxies]Space and Planetary ScienceExperimental High Energy PhysicsActive galaxiesgalaxyAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statistical
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Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

2009

Efficient particle acceleration can modify the structure of supernova remnants. In this context we present the results of the combined analysis of the XMM-Newton EPIC archive observations of SN 1006. We aim at describing the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. We perform a spatially resolved spectral analysis on a set of regions covering the whole rim of the shell and we exploit the results of the spectral analysis to produce a cou…

Astrophysics::High Energy Astrophysical PhenomenaCiencias FísicasFOS: Physical sciencesContext (language use)AstrophysicsISM: individual objects: SN 1006ISM [X-RAYS]//purl.org/becyt/ford/1 [https]ThermalSUPERNOVA REMNANTS [ISM]EjectaISM: supernova remnantAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]X-rays: ISMShock (mechanics)Particle accelerationAstronomíaSupernovaINDIVIDUAL OBJECTS: SN 1006 [ISM]Space and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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X-ray emitting structures in the Vela SNR: ejecta anisotropies and progenitor stellar wind residuals

2021

The Vela supernova remnant (SNR) shows several ejecta fragments protruding beyond the forward shock (shrapnel). Recent studies have revealed high Si abundance in two shrapnel (A and G), located in opposite directions with respect to the SNR center. This suggests the possible existence of a Si-rich jet-counterjet structure. We analyzed an XMM-Newton observation of a bright clump, behind shrapnel G, which lies along the direction connecting A and G. The aim is to study the physical and chemical properties of this clump to ascertain whether it is part of this putative jet-like structure. We produced background-corrected and adaptively-smoothed count-rate images and median photon energy maps, a…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsISM [X-RAYS]Photon energyVela01 natural sciences//purl.org/becyt/ford/1 [https]Protein filamentSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesROSATAstrophysics::Solar and Stellar AstrophysicsSUPERNOVA REMNANTS [ISM]Ejecta010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsISM: supernova remnantsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsVela Supernova Remnant010308 nuclear & particles physicsAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]X-rays: ISMSupernovaISM: individual objects: Vela SNRSpace and Planetary ScienceINDIVIDUAL OBJECTS: VELA SNR [ISM]Astrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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Search for microscopic black holes in a like-sign dimuon final state using large track multiplicity with the ATLAS detector

2013

A search is presented for microscopic black holes in a like-sign dimuon final state in proton-proton collisions at √s= 8 TeV. The data were collected with the ATLAS detector at the Large Hadron Collider in 2012 and correspond to an integrated luminosity of 20.3 fb-1. Using a high track multiplicity requirement, 0.6±0.2 background events from Standard Model processes are predicted and none observed. This result is interpreted in the context of low-scale gravity models and 95% CL lower limits on microscopic black hole masses are set for different model assumptions.

Atlas detectorCiencias FísicasNuclear TheoryHadronDimensions01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Micro black hole[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QANuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsLarge Hadron ColliderLARGE EXTRA DIMENSIONSSettore FIS/01 - Fisica Sperimentaleblack holes; ATLAS detector; microscopicATLASPhysical SciencesLHCParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASNuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Nuclear physics0103 physical sciencesFysikddc:530High Energy PhysicsMultiplicity (chemistry)010306 general physicsCiencias ExactasScience & TechnologyATLAS detector010308 nuclear & particles physicsMillimeterFísica//purl.org/becyt/ford/1.3 [https]black holesAstronomíaBlack holeHADRON-HADRON COLLISIONSExperimental High Energy PhysicsTevPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentGravity SignaturesPHYSICAL REVIEW D
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Search for excited electrons and muons in root s=8 TeV proton-proton collisions with the ATLAS detector

2013

The ATLAS detector at the Large Hadron Collider is used to search for excited electrons and excited muons in the channel pp → ℓℓ* → ℓℓγ, assuming that excited leptons are produced via contact interactions. The analysis is based on 13 fb[superscript −1] of pp collisions at a centre-of-mass energy of 8 TeV. No evidence for excited leptons is found, and a limit is set at the 95% credibility level on the cross section times branching ratio as a function of the excited-lepton mass m[subscript ℓ*]. For m[subscript ℓ*] ≥ 0.8 TeV, the respective upper limits on σB(ℓ* → ℓγ) are 0.75 and 0.90 fb for the e* and μ* searches. Limits on σB are converted into lower bounds on the compositeness scale Λ. In …

Atlas detectorPhysics::Instrumentation and DetectorsCiencias FísicasGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCPhysicsddc:539Excited leptonsLarge Hadron ColliderLepton ProductionSettore FIS/01 - Fisica SperimentaleBranching ratioHERAATLASLarge Hadron ColliderExcited statePhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGQuarkLHCContact interactionExcited electronsParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASQuarkParticle physicsCiências Naturais::Ciências Físicas530 PhysicsParticle physics and field theory:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2excited electrons; muons; proton–proton collisions; ATLAS detector530Nuclear physics0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsCentre-of-mass energiesCiencias ExactasHeraScience & TechnologyMuonATLAS detectorProton proton collisions010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyATLAS detectorsFísica//purl.org/becyt/ford/1.3 [https]AstronomíaHADRON-HADRON COLLISIONSExperimental High Energy PhysicsEp CollisionsHigh Energy Physics::Experimentproton-proton collisionsLepton
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A spatially consistent downscaling approach for SMOS using an adaptive window

2017

The European Space Agency (ESA)'s Soil Moisture and Ocean Salinity (SMOS) is the first spaceborne mission using L-band radiometry to monitor the Earth's global surface soil moisture (SM). After more than 7 years in orbit, many studies have contributed to improve the quality and applicability of SMOS-derived SM maps. In this research, a novel downscaling algorithm for SMOS is proposed to obtain high-resolution (HR) SM maps at 1 km (L4), from the ∼40 km native resolution of the instrument. This algorithm introduces the concept of a shape adaptive moving window as an improvement of the current semi-empirical downscaling approach at SMOS Barcelona Expert Center, based on the “universal triangle…

Atmospheric ScienceBrightnessTeledeteccióMean squared error010504 meteorology & atmospheric sciencesREMEDHUS0211 other engineering and technologiesHigh resolution02 engineering and technology01 natural sciencesNormalized Difference Vegetation IndexBECComputers in Earth SciencesImage resolution021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingNative resolutionAdaptive moving windowLow resolutionMoving windowRemote sensing:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció [Àrees temàtiques de la UPC]Orbit (dynamics)RadiometryEnvironmental scienceSpatial variabilitySoil moistureSòls -- HumitatDownscalingSMOS
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Current and emerging developments in subseasonal to decadal prediction

2020

Weather and climate variations on subseasonal to decadal time scales can have enormous social, economic, and environmental impacts, making skillful predictions on these time scales a valuable tool for decision-makers. As such, there is a growing interest in the scientific, operational, and applications communities in developing forecasts to improve our foreknowledge of extreme events. On subseasonal to seasonal (S2S) time scales, these include high-impact meteorological events such as tropical cyclones, extratropical storms, floods, droughts, and heat and cold waves. On seasonal to decadal (S2D) time scales, while the focus broadly remains similar (e.g., on precipitation, surface and upper-…

Atmospheric ScienceWorld Climate Research Programme010504 meteorology & atmospheric sciencesAtmosfera -- Fenòmens0207 environmental engineeringWeather forecastingInitializationClimate changeWeather and climate02 engineering and technologycomputer.software_genreClimate prediction01 natural sciences//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]MeteorologyHigh-impact meteorological eventsExtratropical cycloneClimate changeMeteorologiaPredictability020701 environmental engineeringdecadal0105 earth and related environmental sciencessubseasonal:Desenvolupament humà i sostenible::Degradació ambiental::Canvi climàtic [Àrees temàtiques de la UPC]Cold wavepredictionClimatic changesExtreme eventsAtmosfera -- Aspectes ambientalsTA13. Climate actionClimatologyWorld Weather Research ProgrammeEnvironmental scienceForecastTropical cyclonecomputerForecastingCanvis climàtics
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Stochastic differential calculus for wind-exposed structures with autoregressive continuous (ARC) filters

2008

In this paper, an alternative method to represent Gaussian stationary processes describing wind velocity fluctuations is introduced. The technique may be considered the extension to a time continuous description of the well-known discrete-time autoregressive model to generate Gaussian processes. Digital simulation of Gaussian random processes with assigned auto-correlation function is provided by means of a stochastic differential equation with time delayed terms forced by Gaussian white noise. Solution of the differential equation is a specific sample of the target Gaussian wind process, and in this paper it describes a digitally obtained record of the wind turbolence. The representation o…

Autoregressive continuous (ARC) modelRenewable Energy Sustainability and the EnvironmentStochastic processMechanical EngineeringGaussianOrnstein–Uhlenbeck processGaussian random fieldStochastic differential equationsymbols.namesakeQuasi-static theoryAutoregressive modelFourier transformsymbolsGaussian functionCalculusStochastic differential calculuApplied mathematicsGaussian random processeSettore ICAR/08 - Scienza Delle CostruzioniGaussian processCivil and Structural EngineeringMathematicsJournal of Wind Engineering and Industrial Aerodynamics
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The Messinian stromatolites of the Sierra del Colmenar (Western Mediterranean): facies characterization and sedimentological interpretation

2018

A representative outcrop of the Messinian stromatolites belonging to the Terminal Carbonate Complex unit, from the northern sector of the Bajo Segura basin (Caja de Ahorros del Mediterraneo section, Sierra del Colmenar, SE Spain) has been studied. Here, we present a detailed analysis of the architecture, external morphology, and internal morphology in order to reconstruct the environmental and palaeoecological conditions for their growth. The stromatolites macrostructure consists of a continuously doming type morphology (build up and sheets areas).These developed close to the coast and acted as a palaeogeographic barrier, reducing physical stress, channeling the erosive effect of water and …

Bajo Segura basinWestern MediterraneanMediterranean climate010506 paleontologyOutcropDominglcsh:MedicineEstratigrafíaMarine BiologyMessinian Salinity CrisisStructural basinGeociencias multidisciplinaria010502 geochemistry & geophysicsNeogene01 natural sciencesGeneral Biochemistry Genetics and Molecular BiologyCiencias de la Tierra y relacionadas con el Medio Ambiente//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]Paleontologychemistry.chemical_compoundStromatolitesCarbonate sedimentologyMicrobial matBajo Segura basin Neogene0105 earth and related environmental sciencesGeneral Neurosciencelcsh:RPaleontologyGeneral MedicineStromatolites Messinian Salinity CrisischemistryFaciesCarbonateTerminal Carbonate ComplexNeogeneGeneral Agricultural and Biological Scienceswestern MediterraneanCIENCIAS NATURALES Y EXACTASGeologyPeerJ
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Esteettisen kritiikki : moderni kokemus ja esteettinen teoria

2008

Ballard J. GkritiikkiAdorno Theodormodernikokemuksetesteettinen teoriaBeckett Samuel
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