Search results for "GAM"

showing 10 items of 5334 documents

Mapping research on legacy of mega sporting events: structural changes, consequences, and stakeholder evaluations in empirical studies

2019

Findings from empirical studies on the legacy of hosting a mega sporting event are inconclusive. This paper considers empirical studies published in English language peer-reviewed journals between ...

Asian gamesHistoryEmpirical researchbusiness.industryEvent (computing)Tourism Leisure and Hospitality ManagementGeography Planning and DevelopmentStakeholderEnglish languagePublic relationsbusinessMega-Leisure Studies
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Historical and Technical Notes on Aqueducts from Prehistoric to Medieval Times

2013

The aim of this paper is to present the evolution of aqueduct technologies through the millennia, from prehistoric to medieval times. These hydraulic works were used by several civilizations to collect water from springs and to transport it to settlements, sanctuaries and other targets. Several civilizations, in China and the Americas, developed water transport systems independently, and brought these to high levels of sophistication. For the Mediterranean civilizations, one of the salient characteristics of cultural development, since the Minoan Era (ca. 3200-1100 BC), is the architectural and hydraulic function of aqueducts used for the water supply in palaces and other settlements. The M…

AspendosEngineeringlcsh:Hydraulic engineeringMinoanBiochimieGeography Planning and DevelopmentWater supplyAqueductGierAquatic ScienceAncient historyBiochemistryPrehistorylcsh:Water supply for domestic and industrial purposeslcsh:TC1-978Human settlementByzantinesPergamonEupalinosStatistique mathématiqueGéographie humaineOcéanographie biologiqueAqua MarciaChinaNimesWater Science and Technologylcsh:TD201-500Aqua claudiaWater transportbusiness.industryAqua marciaProbabilitésKnossosRomansOceanographyValensSalientHellenesCultural developmentAqua ClaudiaSegoviabusinessWater
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Predicting hospital associated disability from imbalanced data using supervised learning.

2019

Hospitalization of elderly patients can lead to serious adverse effects on their functional capability. Identifying the underlying factors leading to such adverse effects is an active area of medical research. The purpose of the current paper is to show the potential of artificial intelligence in the form of machine learning to complement the existing medical research. This is accomplished by studying the outcome of hospitalization of elderly patients as a supervised learning task. A rich set of features characterizing the medical and social situation of elderly patients is leveraged and using confusion matrices, association rule mining, and two different classes of supervised learning algo…

Association rule learningmedicine.medical_treatmentvanhuksetMedicine (miscellaneous)sairaalahoitoOutcome (game theory)Task (project management)03 medical and health sciences0302 clinical medicineArtificial IntelligenceMedicineHumanstoimintarajoitteetDisabled PersonsSet (psychology)Adverse effectFinlandta316030304 developmental biologyAgedta1130303 health sciencesRehabilitationbusiness.industrySupervised learningennusteetta3142medicine.diseaseMedical researchHospitalizationmachine learningkoneoppiminenhospital associated disabilityMedical emergencySupervised Machine Learningtiedonlouhintabusiness030217 neurology & neurosurgeryrandom forestArtificial intelligence in medicine
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Beta Decay Studies of Neutron Rich Nuclei Using Total Absorption Gamma-ray Spectroscopy and Delayed Neutron Measurements

2010

International audience; A complete characterisation of the β-decay of neutron-rich nuclei can be obtained from the measurement of β-delayed gamma rays and, whenever the process is energetically possible, β-delayed neutrons. The accurate determination of the β-intensity distribution and the β-delayed neutron emission probability is of great relevance in the fields of reactor technology and nuclear astrophysics. A programme for combined measurements using the total absorption gamma-ray spectroscopy technique and both neutron counters and neutron time-of-flight spectrometers is presented.

Astrofísica nuclearNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and AstronomyBeta decayNeutron scattering[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesNuclear physicsPrompt neutronNuclear Technology0103 physical sciencesNuclear AstrophysicsNeutron cross sectionNeutronDelayed neutrons emission010306 general physicsNuclear ExperimentSpectroscopyPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Total Absorption Gamma-Rayta114010308 nuclear & particles physicsRadioactivitat betaNeutron stimulated emission computed tomographyBeta DecayDelayed Neutron Emission3. Good healthNeutron Detectors23.40.Bw 29.30.KvNuclear astrophysicsPrompt neutronsDelayed neutronNeutron activation
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Hints of an axion-like particle mixing in the GeV gamma-ray blazar data?

2013

Axion-Like Particles (ALPs), if exist in nature, are expected to mix with photons in the presence of an external magnetic field. The energy range of photons which undergo strong mixing with ALPs depends on the ALP mass, on its coupling with photons as well as on the external magnetic field and particle density configurations. Recent observations of blazars by the Fermi Gamma-Ray Space Telescope in the 0.1-300 GeV energy range show a break in their spectra in the 1-10 GeV range. We have modeled this spectral feature for the flat-spectrum radio quasar 3C454.3 during its November 2010 outburst, assuming that a significant fraction of the gamma rays convert to ALPs in the large scale jet of thi…

AstrofísicaActive galactic nucleusPhotonAxionsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesPartícules (Física nuclear)Spectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBlazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleiRange (particle radiation)Cosmologia010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsQuasarHigh Energy Physics - Phenomenology13. Climate actionAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeJournal of Cosmology and Astroparticle Physics
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Why Have Many of the Brightest Radio-loud Blazars Not Been Detected in Gamma-Rays by Fermi?

2015

We use the complete MOJAVE 1.5 Jy sample of active galactic nuclei (AGNs) to examine the gamma-ray detection statistics of the brightest radio-loud blazars in the northern sky. We find that 23% of these AGNs were not detected above 0.1 GeV by the Fermi-LAT during the four-year 3FGL catalog period partly because of an instrumental selection effect and partly due to their lower Doppler boosting factors. Blazars with synchrotron peaks in their spectral energy distributions located below 10^(13.4) Hz also tend to have high-energy peaks that lie below the 0.1 GeV threshold of the LAT, and are thus less likely to be detected by Fermi. The non-detected AGNs in the 1.5 Jy sample also have significa…

AstrofísicaActive galactic nucleusmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenajets [galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsgeneral [gamma-ray burst]7. Clean energy01 natural scienceslaw.inventionsymbols.namesakelaw0103 physical sciencesBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonPhysicsgeneral [quasars]010308 nuclear & particles physicsScatteringSpectral densityAstronomy and Astrophysicsgalaxies [radio continuum]Synchrotron13. Climate actionSpace and Planetary ScienceSkyactive [galaxies]AstronomiasymbolsDoppler effectFermi Gamma-ray Space Telescope
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Relativistic simulations of black hole-neutron star coalescence: the jet emerges

2014

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of a binary black hole-neutron star on a quasicircular orbit that undergoes merger. The binary mass ratio is 3:1, the black hole initial spin parameter $a/m=0.75$ ($m$ is the black hole Christodoulou mass) aligned with the orbital angular momentum, and the neutron star is an irrotational $\Gamma=2$ polytrope. About two orbits prior to merger (at time $t=t_B$), we seed the neutron star with a dynamically weak interior dipole magnetic field that extends into the stellar exterior. At $t=t_B$ the exterior has a low-density atmosphere with constant plasma parameter $\beta\equiv P_{\rm gas}/P_{\rm mag}$. Varying $\beta$…

AstrofísicaAngular momentumGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsMass ratioPolytropeBlack holeNeutron starSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
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Binary neutron star mergers: a jet engine for short gamma-ray bursts

2016

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of quasi-circular, equal-mass, binary neutron stars that undergo merger. The initial stars are irrotational, $n=1$ polytropes and are magnetized. We explore two types of magnetic-field geometries: one where each star is endowed with a dipole magnetic field extending from the interior into the exterior, as in a pulsar, and the other where the dipole field is initially confined to the interior. In both cases the adopted magnetic fields are initially dynamically unimportant. The merger outcome is a hypermassive neutron star that undergoes delayed collapse to a black hole (spin parameter $a/M_{\rm BH} \sim 0.74$) imme…

AstrofísicaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyArticlePulsar0103 physical sciencesBinary starAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsBlack holeNeutron starStarsSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaMagnetic dipole
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The Gamma-Ray Emitting Radio-Loud Narrow-Line Seyfert 1 Galaxy PKS 2004-447 II. The Radio View

2015

Gamma-ray detected radio-loud narrow-line Seyfert 1 (g-NLS1) galaxies constitute a small but interesting sample of the gamma-ray loud AGN. The radio-loudest g-NLS1 known, PKS 2004-447, is located in the southern hemisphere and is monitored in the radio regime by the multiwavelength monitoring program TANAMI. We aim for the first detailed study of the radio morphology and long-term radio spectral evolution of PKS 2004-447, which are essential to understand the diversity of the radio properties of g-NLS1s. The TANAMI VLBI monitoring program uses the Australian Long Baseline Array (LBA) and telescopes in Antarctica, Chile, New Zealand, and South Africa to monitor the jets of radio-loud active …

AstrofísicaBrightnessActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral line0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsSpectral componentMonitoring programGalaxySpace and Planetary ScienceComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstronomiaAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space Telescope
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Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

2016

Using high-resolution radio imaging with VLBI techniques, the TANAMI program has been observing the parsec-scale radio jets of southern (declination south of -30{\deg}) gamma-ray bright AGN simultaneously with Fermi/LAT monitoring of their gamma-ray emission. We present the radio and gamma-ray properties of the TANAMI sources based on one year of contemporaneous TANAMI and Fermi/LAT data. A large fraction (72%) of the TANAMI sample can be associated with bright gamma-ray sources for this time range. Association rates differ for different optical classes with all BL Lacs, 76% of quasars and just 17% of galaxies detected by the LAT. Upper limits were established on the gamma-ray flux from TAN…

AstrofísicaBrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationRadio continuum: galaxies0103 physical sciencesVery-long-baseline interferometryGalaxies; Interferometry; Luminance; Radio astronomy; Temperature Galaxies : active; Galaxies: nuclei; Galaxies:jets; Gamma rays: galaxies; Radio continuum: galaxies Gamma rays; Galaxies: active; Galaxies: jets; Galaxies: nuclei; Gamma rays: galaxies; Radio continuum: galaxiesRadio astronomyBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxies: nuclei0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGalaxies : activeGalaxies:jetsGamma raysTemperatureGamma rayAstronomy and AstrophysicsQuasarGalaxies: activeGalaxiesGalaxyGamma rays: galaxiesInterferometryLuminanceGalaxies: jetsSpace and Planetary ScienceAstronomiaComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeAstronomy & Astrophysics
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