Search results for "likelihood"

showing 10 items of 264 documents

A novel family of tRNA-derived SINEs in the colugo and two new retrotransposable markers separating dermopterans from primates.

2003

Abstract Short interspersed nuclear elements (SINEs) provide a near homoplasy free and copious source of molecular evolutionary markers with precisely defined character polarity. Used as molecular cladistic markers in presence/absence analyses, they represent a powerful complement to phylogenetic reconstructions that are based on sequence comparisons on the level of nucleotide substitutions. Recent sequence comparisons of large data sets incorporating a broad eutherian taxonomic sample have led to considerations of the different primate infraorders to constitute a paraphyletic group. Statistically significant support against the monophyly of primates has been obtained by clustering the flyi…

ParaphylyGeneticsMammalsLikelihood FunctionsbiologyPhylogenetic treeBase SequenceMolecular Sequence Databiology.organism_classificationCladisticsColugoEvolution MolecularMonophylySister groupRNA Transferbiology.animalGeneticsAnimalsPrimateCynocephalus variegatusMolecular BiologyEcology Evolution Behavior and SystematicsPhylogenyDNA PrimersShort Interspersed Nucleotide ElementsMolecular phylogenetics and evolution
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Graphical models for estimating dynamic networks

2012

Het bepalen van dynamische netwerken met behulp van data is een actief onderzoeksgebied, met name in de systeem biologie. Het schatten van de structuur van een netwerk heeft te maken met het bepalen van de aan of afwezigheid van een relatie tussen de hoekpunten in de graaf. Grafische modellen definiëren deze relaties via conditionele afhankelijkheid. In Gaussiaanse grafische modellen (GGM) wordt verondersteld dat de hoekpunten een normale verdeling volgen. Dit heeft grote voordelen vanwege de computationele handelbaarheid van GGM. Standaard GGM zijn echter niet bruikbaar om grote netwerken te bestuderen, i.e. als het aantal waarnemingen minder is dan het aantal hoekpunten van de graaf. Rece…

Penalized Likelihood Graphical Models Dynamic Networks State-space modelDynamische modellenLatent VariablesNetwerkenmathematische statistiekgraphical modelestimating dynamic networks.Proefschriften (vorm)Settore SECS-S/01 - StatisticaNormale verdelingDynamische systemenSysteembiologieGrafische methoden
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Penalized inference in multivariate ordered logistic models: theory and applications

2010

Penalized LikelihoodSettore SECS-S/01 - StatisticaMultivariate Logistic Model
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User participation in knowledge update of expert systems

1997

Abstract Applying the Elaboration Likelihood Model (ELM) of persuasion we conducted an experiment to examine the effect of participation of users in the design process on their acceptance of system recommendations and revision of their original decisions. Results of our study indicate that two different types of information processing occur when subjects are reviewing the expert system recommendations. 1. (i) For users who have a high perceived level of participation in updating the knowledge of the ES, ambiguity of the decision setting is the primary determinant affecting acceptance of the recommendation from the ES. 2. (ii) For users who have a low perceived level of participation in upda…

PersuasionEngineeringInformation Systems and ManagementKnowledge managementbusiness.industrymedia_common.quotation_subjectInformation processingUser participationAmbiguitycomputer.software_genreExpert systemManagement Information SystemsSubject-matter expertbusinessEngineering design processcomputerInformation Systemsmedia_commonElaboration likelihood modelInformation & Management
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Estimating the angular resolution of tracks in neutrino telescopes based on a likelihood analysis

2004

A semianalytic method to estimate the angular resolution of tracks, that have been reconstructed by a likelihood approach, is presented. The optimal choice of coordinate systems and resolution parameters, as well as tests of the method are discussed based on an application for a neutrino telescope.

PhysicsAstrophysics (astro-ph)Coordinate systemNeutrino telescopeResolution (electron density)ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysicsComputational physicsLikelihood analysisNeutrino detectorMeasurements of neutrino speedAngular resolutionNeutrinoAstroparticle Physics
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A Robust Determination of the size of quasar accretion disks using gravitational microlensing

2012

Using microlensing measurements from a sample of 27 image-pairs of 19 lensed quasars we determine a maximum likelihood estimate for the accretion disk size of an {{\em}average} quasar of $r_s=4.0^{+2.4}_{-3.1} $ light days at rest frame $=1736$\AA\ for microlenses with a mean mass of $=0.3M_\odot$. This value, in good agreement with previous results from smaller samples, is roughly a factor of 5 greater than the predictions of the standard thin disk model. The individual size estimates for the 19 quasars in our sample are also in excellent agreement with the results of the joint maximum likelihood analysis.

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsMaximum likelihoodFOS: Physical sciencesAstronomy and AstrophysicsQuasarMaximum likelihood analysisAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRest frameGravitational microlensing01 natural sciencesAccretion discThin diskSpace and Planetary Science0103 physical sciencesAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Approches région et bayésienne pour la restauration ďimages dégradées par la turbulence atmosphérique

2001

La turbulence atmospherique perturbe ľobservation a haute resolution. C’est un phenomene etudie depuis longtemps, en astronomie notamment. Le present article porte sur le cas de ľobservation ďun objet situe environ vingt kilometres, la propagation etant horizontale et pres du sol, en infrarouge. Les images a longue pose sont restaurees avec des algorithmes classiques de deconvolution. Les resultats ne sont satisfaisants que pour une faible perturbation. Il est plus avantageux ďexploiter des images courte pose, car elles contiennent plus de hautes frequences spatiales; mais ľobjet observe y fluctue aleatoirement. On travaille donc ici partir ďune sequence de plusieurs dizaines ďimages. Deux …

PhysicsMaximum likelihoodAtmospheric turbulenceElectrical and Electronic EngineeringHumanitiesComputer communication networksAnnales Des Télécommunications
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Measurements of neutralBdecay branching fractions toKS0π+π−final states and the charge asymmetry ofB0→K*+π−

2006

Branching fraction measurements using B-meson decays to Kspi+pi- are presented. These measurements were obtained by analyzing a data sample of 88.9 million Y(4S) --> BB decays collected with the BaBar detector at the SLAC PEP-II asymmetric-energy B factory. Using a maximum likelihood fit, the following branching fraction results were obtained: Br(B0 -> K0pi+pi- = (43.7 +/- 3.8 +/- 3.4) * 10^-6, Br(B0 --> K{*+}pi-) = (12.9 +/- 2.4 +/- 1.4) * 10$^-6} and Br(B0 --> D-(--> Kspi-)pi+ = (42.7 +/- 2.1 +/- 2.2) * 10^{-6}. The CP violating char ge asymmetry A(K*pi} for the decay B0 --> $K{*+}pi-$ was measured to be A(K*pi} = 0.23 +/- $0.18^{+0.09}_{-0.06}$. For all these measurements the first error…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsBranching fractionmedia_common.quotation_subjectMaximum likelihoodAnalytical chemistryBranching (polymer chemistry)01 natural sciencesAsymmetryParticle identificationB-factoryNuclear physicsParticle decay0103 physical sciencesPi010306 general physicsmedia_commonPhysical Review D
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Searching for localized cosmic particle sources with an unbinned maximum likelihood approach

2006

Abstract An unbinned method to search for localized cosmic particle sources is presented. The expected source shape, the measured background shape, and the estimated angular resolution of individual tracks are used to construct a likelihood function. Estimates of the flux, the position and—in particular—the significance of a source can be readily obtained. A full confidence belt construction to deduce flux limits is presented. General statistical issues when searching for sources of unknown position are discussed.

PhysicsNuclear and High Energy PhysicsCOSMIC cancer databaseLikelihood analysisPosition (vector)Maximum likelihoodFluxParticleAngular resolutionAstrophysicsStatistical physicsLikelihood functionInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Precision measurement of the mass of the tau lepton

2014

An energy scan near the $\tau$ pair production threshold has been performed using the BESIII detector. About $24$ pb$^{-1}$ of data, distributed over four scan points, was collected. This analysis is based on $\tau$ pair decays to $ee$, $e\mu$, $eh$, $\mu\mu$, $\mu h$, $hh$, $e\rho$, $\mu\rho$ and $\pi\rho$ final states, where $h$ denotes a charged $\pi$ or $K$. The mass of the $\tau$ lepton is measured from a maximum likelihood fit to the $\tau$ pair production cross section data to be $m_{\tau} = (1776.91\pm0.12 ^{+0.10}_{-0.13}$) MeV/$c^2$, which is currently the most precise value in a single measurement.

PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilation010308 nuclear & particles physicshep-exElectron–positron annihilationMaximum likelihoodSingle measurementDetectorBESIII01 natural sciencesDECAYSHigh Energy Physics - ExperimentNuclear physicsENERGYPair production0103 physical sciencesRADIATIVE-CORRECTIONSHigh Energy Physics::Experiment010306 general physicsANNIHILATIONDETECTORSYSTEMLepton
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