Search results for "Mill"

showing 10 items of 950 documents

Some awkward issues on pairwise comparison matrices

2017

Many decision-making techniques use pairwise comparisons (PCs) elicited by one or more stakeholders involved in a given corresponding decision-making process. In very complex problems, the number of criteria or options to be compared may be too large, thus limiting PC applicability to large-scale decision problems due to the so-called curse of dimensionality, that is, a large number of pairwise comparisons need to be produced from a decision maker. For example, in AHP, Saaty [1] recommends that to obtain a reasonable and consistent PC matrix, the number of comparing elements should be at most seven. In [2] and [3], arguing on limitations of the human capabilities, the maximum number of elem…

AHPwater distribution system (WDS)management and operation of a WDSMiller’s magic number sevenpairwise comparisondecision-making
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María Magdalena. Continuidad y variación en la cultura audiovisual (1897-2014)

2017

El objetivo principal de esta tesis consiste en analizar la presencia de María Magdalena en las producciones audiovisuales del periodo comprendido entre 1897 y 2014. Dichas producciones proceden de Europa, Estados Unidos, Canadá y México. El marco metodológico general a partir del que se plantea el análisis es la iconología, entendida como Zwichenraum o tierra de confluencias. En concreto, la noción de continuidad y variación, iniciada por Aby Warburg y continuada por Fritz Saxl, es la principal cuestión teórica en la que se basa la aproximación. El estudio se lleva a cabo en perspectiva diacrónica con el objetivo de detectar dichas fases de continuidad y variación del personaje a lo largo …

Aby WarburgPier Paolo PassoliniMel GibsonPanofsky:HISTORIA [UNESCO]Franco ZeffirelliIconografía e iconologíaPeter Mullan:PEDAGOGÍA::Teoría y métodos educativos::Medios audiovisuales [UNESCO]feminismoscultura audiovisualUNESCO::HISTORIAcinereligiónUNESCO::PEDAGOGÍA::Teoría y métodos educativos::Medios audiovisualesiconografía e iconologíaFeminismosJules Dassinestudios culturalesMaría MagdalenaIgnacio F. Iquinocultura visualStuart HallFritz SaxlMusicalReligiónRichard JohnsoncómicArthur MaudeLady GagaUNESCO::HISTORIA::Historia por especialidades::Historia del arteInterdisciplinariedadteología feministaWerner HerzogvideoclipEstudios comparativosDenys ArcandTipos iconográficosMartin ScorseseRobert WieneNicholas RayMiguel Contreras Torrescontinuidad y variaciónliteraturaNikos KazantzakisanimeCecil B. DeMilleestudios de género:HISTORIA::Historia por especialidades::Historia del arte [UNESCO]
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Spectral changes during six years of Scorpius X-1 monitoring with BeppoSAX Wide Field Cameras

2005

We analyse a sample of fifty-five observations of Scorpius X-1 available in the BeppoSAX Wide Field Camera public archive and spanning over the six years of BeppoSAX mission life. Spectral changes are initially analysed by inspection of colour-colour and colour-intensity diagrams, we also discuss the shift of the Z tracks in these diagrams. Then we select two long observations for spectral fitting analysis, a secular shift is evident between the tracks in these observations. We finally extract spectra along the tracks and discuss the best fit model, the parameter variations along the track and between tracks, and their link to the accretion rate.

Accretion (meteorology)Track (disk drive)Astrophysics (astro-ph)X-ray binaryFOS: Physical sciencesAstrophysicsX-ray neutron stars accreting millisecondAstrophysicsWide fieldSpectral lineAccretion rateNeutron starSpectral fittingGeologyAIP Conference Proceedings
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Pulsating in Unison at Optical and X-Ray Energies: Simultaneous High Time Resolution Observations of the Transitional Millisecond Pulsar PSR J1023+00…

2019

PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an accretion disk and also showed X-ray pulsations. We report on the first high time resolution observational campaign of this transitional pulsar in the disk state, using simultaneous observations in the optical (TNG, NOT, TJO), X-ray (XMM-Newton, NuSTAR, NICER), infrared (GTC) and UV (Swift) bands. Optical and X-ray pulsations were detected simultaneously in the X-ray high intensity mode in which the source spends $\sim$ 70% of the time, and both disappeared in the low mode, indicating a common underlying physical mechanism. In addition, o…

AccretionAccretion disks-pulsars: Individual (psr j1023+0038)-stars: Neutron-X-rays: Binaries010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarAccretion discMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsX-rayAstronomy and AstrophysicsTime resolutionAccretion (astrophysics)Space and Planetary ScienceVisible bandAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Broad-band spectral analysis of the accreting millisecond X-ray pulsar SAX J1748.9-2021

2016

We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021. The source showed numerous type-I burst episodes during the XMM-Newton observation, and for this reason we studied separately the persistent and burst epochs. We described the persistent emission with a combination of two soft thermal components, a cold thermal Comptonization component (~2 keV) and an additional hard X-ray emission described by a power-law (photon index ~2.3). The continuum components can be associated with an accretion disc, the neutron star (NS) surface and a thermal Compton…

AccretionBinaries - X-rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesIndividualAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSAX J1748.9-2021Millisecond pulsarAccretion discs -X-ray0103 physical sciencesAccretion; Accretion discs -X-rays; Binaries - X-rays; Galaxies -X-rays; Individual; SAX J1748.9-2021; Space and Planetary Science; Astronomy and Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSolar massMillisecondAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceGalaxies -X-rayEddington luminositysymbolsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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Timing of the accreting millisecond pulsar IGR J17591-2342: evidence of spin-down during accretion

2020

We report on the phase-coherent timing analysis of the accreting millisecond X-ray pulsar IGR J17591-2342, using Neutron Star Interior Composition Explorer (NICER) data taken during the outburst of the source between 2018 August 15 and 2018 October 17. We obtain an updated orbital solution of the binary system. We investigate the evolution of the neutron star spin frequency during the outburst, reporting a refined estimate of the spin frequency and the first estimate of the spin frequency derivative ($\dot{\nu} \sim -7\times 10^{-14}$ Hz s$^{-1}$), confirmed independently from the modelling of the fundamental frequency and its first harmonic. We further investigate the evolution of the X-ra…

AccretionIGR J17591-2342Astrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesaccretion accretion disc stars: neutron X-rays: binaries010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron Star Interior Composition Explorer010308 nuclear & particles physicsAstronomy and Astrophysicsneutron [Stars]Accretion (astrophysics)Magnetic fieldNeutron starAmplitudeSpace and Planetary Sciencebinaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsAccretion discAstrophysics - High Energy Astrophysical Phenomena
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A Hard X-Ray View of Scorpius X-1 with INTEGRAL : Nonthermal Emission?

2006

We present here simultaneous INTEGRAL/RXTE observations of Sco X-1, and in particular a study of the hard X-ray emission of the source and its correlation with the position in the Z-track of the X-ray color-color diagram. We find that the hard X-ray (above about 30 keV) emission of Sco X-1 is dominated by a power-law component with a photon index of ~3. The flux in the power-law component slightly decreases when the source moves in the color-color diagram in the sense of increasing inferred mass accretion rate from the horizontal branch to the normal branch/flaring branch vertex. It becomes not significantly detectable in the flaring branch, where its flux has decreased by about an order of…

AccretionPhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciencesneutron starsX-ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Position (vector)Accretion DisksStars: Neutron0103 physical sciencesX-Rays: StarsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)DiagramAstronomy and AstrophysicsSense (electronics)Horizontal branchX-Rays: BinariesX-Rays: GeneralSpace and Planetary ScienceVertex (curve)accreting millisecondStars: Individual: Constellation Name: Scorpius X-1Order of magnitudeThe Astrophysical Journal
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Accuracy assessment and position correction for low-cost non-differential GPS as applied on an industrial peat bog

1999

A low-cost, non-differentially corrected hand-held GPS receiver was tested on an industrial peat production bog. A correction procedure (‘pseudo-differential correction’) was derived that corrected data points to the nearest position on a line defining the centre of each 15-m wide field. The result was a corrected log of track points for each field for all points lying along the field. It was found that the mean orthogonal distance from a field centreline was linearly correlated with mean uncorrected GPS data error (r 2 0.99) such that as GPS error increased so the accuracy obtained by correction decreased. For a signal with a mean uncorrected error of 30 m it was possible to reduce the err…

Accuracy and precisionPeatbusiness.industryGPSSettore AGR/09 - Meccanica AgrariaForestryMilled peatHorticultureError analysis for the Global Positioning SystemComputer Science ApplicationsData pointPositioning accuracyGlobal Positioning SystemDifferential correctionPositioning accuracy; GPS; Differential correction; Milled peatEnergy sourceDifferential GPSbusinessAgronomy and Crop ScienceEnergy (signal processing)MathematicsRemote sensing
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Jeux et enjeux du paraître lors de l'entrée en cours préparatoire et de l'entrée en sixième

1993

International audience

Accès à l'enseignement primaire[SHS.EDU]Humanities and Social Sciences/Education[SHS.EDU] Humanities and Social Sciences/EducationRelation famille-écoleFamillePratiqueEntrée en 6emeAccès à l'enseignement secondaireComputingMilieux_MISCELLANEOUSApparence physique
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Acute Effects on Impact Accelerations Running with Objects in the Hand

2021

Amateur runners usually run carrying implements in their hands (keys, a mobile phone, or a bottle of water). However, there is a lack of literature about the effects of different handloads on impact accelerations. Thus, this study aimed to analyse the effects of carrying different objects in the hand on impact accelerations during running. Nineteen male recreational runners (age 24.3 ± 6.8 years, training volume of 25 ± 7.38 km/week) performed twenty minutes of running on a treadmill at 2.78 m/s with four different conditions: no extra weight, with keys, with a mobile phone, and with a bottle of water. Impact acceleration and spatio-temporal parameters were analysed through a wireless triax…

Acute effectsmedicine.medical_specialtyimpact accelerationsSciencerunSTRIDEasymmetric handloadsAccelerometerGeneral Biochemistry Genetics and Molecular BiologyArticle03 medical and health sciencesAcceleration0302 clinical medicinePhysical medicine and rehabilitationmedicineEducación Física y DeportivaTreadmillspatio-temporal parametersEcology Evolution Behavior and SystematicsMathematicsImpact accelerationAsymmetric handloadsRunQImpact accelerationsSpatio-temporal parametersPaleontology030229 sport sciencesShock (mechanics)Space and Planetary ScienceMobile phone030217 neurology & neurosurgeryLife
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