Search results for "Gram"

showing 10 items of 9069 documents

A. Socins Arabische Grammatik: Paradigmen, Literatur, Übungsstücke und Glossar

1909

Teksts vācu un arābu valodā, titullapa vācu valodā.

Arābu valoda - gramatika:HUMANITIES and RELIGION::Languages and linguistics::Other languages::Arabic language [Research Subject Categories]Arabic grammarArabische Grammatik
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The Linguistic Roots of Gramsci's Non-Marxism

2010

AscoliMarxismoGramsciEgemoniaLinguaggioManzoniSettore M-FIL/05 - Filosofia E Teoria Dei Linguaggi
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Solving type-2 Assembly Line Balancing Problem with Fuzzy Binary Linear Programming

2013

Assembly Line Balancing Problem Fuzzy Binary Linear ProgrammingAssembly Line Balancing Problem; Fuzzy Binary Linear Programming
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Human factor policy testing in the sequencing of manual mixed model assembly lines

2004

In this paper the human resource management in manual mixed model assembly U-lines is considered. The objective is to minimise the total conveyor stoppage time to achieve the full efficiency of the line. A model, that includes effects of the human resource, was developed in order to evaluate human factor policies impact on the optimal solution of this line sequencing problem. Different human resource management policies are introduced to cope with the particular layout of the proposed line. Several examples have been proposed to investigate the effects of line dimensions on the proposed management policies. The examples have been solved through a genetic algorithm. The obtained results conf…

Assembly line; Conveyor stoppage; Human factor; SequencingMixed modelConveyor stoppageMathematical optimizationGeneral Computer ScienceOperations researchComputer sciencebusiness.industryAssembly lineManagement Science and Operations ResearchSettore ING-IND/35 - Ingegneria Economico-GestionaleModeling and SimulationHuman resource managementFactor (programming language)Human factorGenetic algorithmSequencingLine (text file)Human resourcesbusinesscomputercomputer.programming_language
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Models of E-Democracy

2006

Pulished article in Communications of the Association for Information Systems, 17 (1), 818-840. Also available from the publisher: http://aisel.aisnet.org/cais/vol17/iss1/37/ Several theories of E-Democracy have been presented, and implementations of and experiments in E-Democracy emerged. However, existing literature on the subject appears rather non-comprehensive, lacking an integrated basis, for gathering knowledge in the future. After an analysis of theories of E-Democracy versus implementations reported in related literature, we address the need for a model generally absent from contemporary theoretical literature: the Partisan model of E-Democracy. We aim to simplify the current "jung…

Association (object-oriented programming)Political scienceE-Democracy democracy models literature reviewInformation systemVDP::Social science: 200::Library and information science: 320::Information and communication systems: 321Social scienceE-democracyInformation SystemsPeer review
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The gamma-ray emitting radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447 I. The X-ray View

2015

As part of the TANAMI multiwavelength progam, we discuss new X-ray observations of the $\gamma$-ray and radio-loud Narrow Line Seyfert galaxy ($\gamma$-NLS1) PKS 2004-447. The active galaxy is a member of a small sample of radio-loud NLS1s detected in $\gamma$-rays by the Fermi Large Area Telescope. It is the radio-loudest and only southern-hemisphere source in this sample. We present results from our X-ray monitoring program comprised of Swift snapshot observations from 2012 through 2014 and two new X-ray observations with XMM-Newton in 2012. We analyze the X-ray spectrum and variability of this peculiar source using supplementary archival data from 2004 and 2011. The (0.5-10) keV spectrum…

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumlaw.inventionTelescopeRelativistic beaminglaw0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsMonitoring programAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)AstronomiaComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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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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The Gaia-ESO Survey: Chromospheric emission, accretion properties, and rotation in gamma Velorum and Chamaeleon

2015

Aims: One of the goals of the Gaia-ESO Survey (GES), which is conducted with FLAMES at the VLT, is the census and the characterization of the low-mass members of very young clusters and associations. We conduct a comparative study of the main properties of the sources belonging to γ Velorum (γ Vel) and Chamaeleon I (Cha I) young associations, focusing on their rotation, chromospheric radiative losses, and accretion. Methods: We used the fundamental parameters (effective temperature, surface gravity, lithium abundance, and radial velocity) delivered by the GES consortium in the first internal data release to select the members of γ Vel and Cha I among the UVES and GIRAFFE spectroscopic obser…

Astrofísicastars: chromospheresAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRotationStars: chromosphereOpen clusters and associations: individual:γVelorumstars: low-massStars: low-maAstrophysics::Solar and Stellar AstrophysicsOpen clusters and associations: individual: Chamaeleon Iopen clusters and associations: individual: γ VelorumQCAstrophysics::Galaxy AstrophysicsQBLine (formation)PhysicsAccretion (meteorology)stars: chromospheres ; stars: low-mass; open clusters and associations: individual: γ VelorumDiagramStars: rotationSpectral densityAstronomy and AstrophysicsAstronomy and AstrophysicStarsDistribution (mathematics)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceChamaeleonStars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen clusters and associations: individual: Chamaeleon I; Open clusters and associations: individual:γVelorum; Stars: chromospheres; Stars: low-mass; Stars: pre-main sequence; Stars: rotation
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Zvaigžņotā Debess: 2016/17, Ziema (234)

2016

Contents: “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: A.Balklavs. New Possibilities in Search of Cosmic Gravitational Waves (abridged) ; E.Mūkins. «Venus-9» and «Venus-10» Scientific Accomplishment (abridged) ; DEVELOPMENTS in SCIENCE: K.Schwartz. The Unknown Solar Corona ; DISCOVERIES: I.Pundure. Gaia Has Obtained Billion-Star 3D Map ; SPACE RESEARCH and EXPLORATION: J.Jaunbergs. Tar Lakes of Titan ; R.Misa. A Step Closer to Stars ; CONFERENCES and MEETINGS: J.Balodis. Copernicus Is Becoming an Impressive Business ; K.Bērziņš. Conference of Young European Radioastronomers at the Latvian Centre in Germany ; FLASHBACK: A.Alksnis. Short Trips and Faraway Journeys (concluded) ; For SCHOOL YOUTH: D.Bo…

Astroloģija-pareģojumiESA Copernicus programmaLVU astronomijas studenti – vēstulesLatvijas 41.atklātā fizikas olimpiāde16.astronomijas amatieru salidojums Starspace observatorijā:NATURAL SCIENCES::Physics::Astronomy and astrophysics [Research Subject Categories]LU Astronomijas institūts 2015.gadāSaules aptumsumi filatēlijāMildai Zepei – 100“Zvaigžņotās Debess” autori – pasākums Latvijas Zinātņu akadēmijāMārtiņam Bucleram – 150Debess spīdekļi – 2016. gada rudensAstroloģija – astromaģijaEiropas jaunie radioastronomi latviešu centrā BonnāStarpzvaigžņu zonde StarChipZvaigžņu svītru fotogrāfijasSaules koronaGaia’s pirmais katalogs – miljardzvaigžņu 3D karteLatvijas līgums ar CERNValfrīdam Osvaldam – 100Titāns – darvas ezeriPilns Saules aptumsums Sulavesi salāSaules pulksteņi Latvijā 2011-2015Saules pulksteni Latvijas simtgadei
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The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

2021

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operati…

AstronomyLarge detector systems for particle and astroparticle physics; Optics; Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Real-time monitoringReal-time monitoring01 natural sciencesAugerSuccessful operationObservatoryopticalAPDshardwareAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsInstrumentationPhoton detectors for UVMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEEBCCDsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsAugerobservatoryRobotic telescopeG-APDsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSciences exactes et naturellesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesprogrammingdetector: fluorescencePhotometry (optics)0103 physical sciencesddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Physicsvisible and IR photons (solid-state) (PIN diodesCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingetc)fluorescence [detector]Pierre Auger Observatory010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsActive monitoringOpticsCCDslasermonitoringEMCCDsLarge detector systems for particle and astroparticle physicatmosphereExperimental High Energy PhysicsOpticEnvironmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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