Search results for "Large"

showing 10 items of 2197 documents

Morphostatistical characterization of the spatial galaxy distribution through Gibbs point processes

2021

This paper proposes a morpho-statistical characterisation of the galaxy distribution through spatial statistical modelling based on inhomogeneous Gibbs point processes. The galaxy distribution is supposed to exhibit two components. The first one is related to the major geometrical features exhibited by the observed galaxy field, here, its corresponding filamentary pattern. The second one is related to the interactions exhibited by the galaxies. Gibbs point processes are statistical models able to integrate these two aspects in a probability density, controlled by some parameters. Several such models are fitted to real observational data via the ABC Shadow algorithm. This algorithm provides …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)InferenceFOS: Physical sciencesProbability density functionAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPoint processmethods: numerical010104 statistics & probability0103 physical sciencesStatistical physics0101 mathematics010303 astronomy & astrophysicscataloguesgalaxies: statisticsPhysics[STAT.AP]Statistics [stat]/Applications [stat.AP]methods: statisticalEstimation theoryAstronomy and AstrophysicsStatistical modelmethods: data analysisField (geography)GalaxyDistribution (mathematics)Space and Planetary Sciencelarge-scale structure of Universe[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Galaxy clusters and groups in the ALHAMBRA survey

2015

Ascaso, Begoña et al.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of UniverseFOS: Physical sciencesAstrophysicsX-rays galaxies clustersclusters: general [Galaxies]Galaxies clusters generalobservations [Cosmology]Galaxy clusterPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Cosmology: observationsFísicaAstronomyGalaxies: evolutionAstronomy and Astrophysicsevolution [Galaxies]Cosmology observationsCataloguesGalaxies evolutionSpace and Planetary Science[SDU]Sciences of the Universe [physics]X-rays: galaxies: clustersgalaxies: clusters [X-rays]Galaxies: clusters: generalAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark matter results from 225 live days of XENON100 data

2012

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit o…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsLarge Underground Xenon experimentDark matterFOS: Physical sciencesGeneral Physics and AstronomyWIMP Argon Programme01 natural sciences7. Clean energyParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsLiquid XenonPhysicsRange (particle radiation)010308 nuclear & particles physicsDARK MATTERInstrumentation and Detectors (physics.ins-det)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DAMA/NaITPCPandaXDirect search for Dark MatterAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

2021

Stanford, S. A., et al.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Calibration (statistics)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor space217101 natural sciencesCosmologyLarge-scale structure010309 optics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]galaxy spectroscopySettore FIS/05 - Astronomia e AstrofisicaSpitzer Space Telescope0103 physical sciencesDISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics::Galaxy AstrophysicsPhysicsHardware_MEMORYSTRUCTURESAstrophysics::Instrumentation and Methods for AstrophysicsEuclidAstronomy and AstrophysicsRedshiftGalaxyCosmologySpace and Planetary ScienceGalaxy spectroscopyDark energyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Nonlinear dynamical model of Costas loop and an approach to the analysis of its stability in the large

2015

The analysis of the stability and numerical simulation of Costas loop circuits for highfrequency signals is a challenging task. The problem lies in the fact that it is necessary to simultaneously observe very fast time scale of the input signals and slow time scale of phase difference between the input signals. To overcome this difficult situation it is possible, following the approach presented in the classical works of Gardner and Viterbi, to construct a mathematical model of Costas loop, in which only slow time change of signal's phases and frequencies is considered. Such a construction, in turn, requires the computation of phase detector characteristic, depending on the waveforms of the…

Costas loopphase detector characteristicstability in the largenonlinear analysisphase comparatorsimulointiphase-locked loop (PLL)BPSK
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Nonlinear dynamical model of Costas loop and an approach to the analysis of its stability in the large

2015

The analysis of the stability and numerical simulation of Costas loop circuits for high-frequency signals is a challenging task. The problem lies in the fact that it is necessary to simultaneously observe very fast time scale of the input signals and slow time scale of phase difference between the input signals. To overcome this difficult situation it is possible, following the approach presented in the classical works of Gardner and Viterbi, to construct a mathematical model of Costas loop, in which only slow time change of signal?s phases and frequencies is considered. Such a construction, in turn, requires the computation of phase detector characteristic, depending on the waveforms of th…

Costas loopta213phase detector characteristicstability in the largeta111phase comparatorsimulationPhase detectorphase-locked loop (PLL)Loop (topology)Phase-locked loopNonlinear systemControl and Systems EngineeringControl theoryCostas loopPhase spaceSignal Processingnonlinear analysisPhase detector characteristicComputer Vision and Pattern RecognitionLinear approximationElectrical and Electronic EngineeringSoftwareBPSKMathematicsSignal Processing
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Limits on anomalous trilinear gauge boson couplings from WW, WZ and Wγ production in pp¯ collisions at s=1.96 TeV

2012

We present searches for the anomalous γWW and ZWW trilinear gauge boson couplings from WW and WZ production using lepton plus dijet final states and a combination with results from Wγ, WW, and WZ production with leptonic final states. The analyzed data correspond to up to 8.6fb -1 of integrated luminosity collected by the D0 detector in pp- collisions at s=1.96TeV. We set the most stringent limits at a hadron collider to date assuming two different relations between the anomalous coupling parameters δκ γ, λ, and δg1Z for a cutoff energy scale Λ=2TeV. The combined 68% C.L. limits are -0.057lδκ γl0.154, -0.015lλl0.028, and -0.008lδg1Zl0.054 for the LEP parameterization, and -0.007lδκl0.081 an…

CouplingPhysicsNuclear and High Energy PhysicsParticle physicsGauge bosonLuminosity (scattering theory)Large Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenology01 natural sciences7. Clean energyNuclear physics0103 physical sciencesQuadrupoleCutoffHigh Energy Physics::Experiment010306 general physicsMagnetic dipoleLeptonPhysics Letters B
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Top quark anomalous tensor couplings in the two-Higgs-doublet models

2013

We compute the one loop right and left anomalous tensor couplings (g(R) and g(L), respectively) for the top quark, in the aligned two-Higgs-doublet model. They are the magnetic-like couplings in the most general parameterization of the tbW vertex. We find that the aligned two-Higgs doublet model, that includes as particular cases some of the most studied extensions of the Higgs sector, introduces new electroweak contribution's and provides theoretical predictions that are very sensitive to both new scalar masses and the neutral scalar mixing angle. For a largo area in the parameters space we obtain significant deviations in both the real and the imaginary parts of the couplings gR and gL, c…

CouplingPhysicsNuclear and High Energy PhysicsParticle physicsTop quarkStandard ModelLarge Hadron ColliderPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyElectroweak interactionFísicaFOS: Physical sciencesHiggs sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Beyond Standard ModelHiggs bosonCP violationJournal of High Energy Physics
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Experimental constraints on the coupling of the Higgs boson to electrons

2015

In the standard model (SM), the coupling of the Higgs boson to electrons is real and very small, proportional to the electron mass. New physics could significantly modify both real and imaginary parts of this coupling. We discuss experiments which are sensitive to the Higgs-electron coupling and derive the current bounds on new physics contributing to this coupling. The strongest constraint follows from the ACME bound on the electron electric dipole moment (EDM). We calculate the full analytic two-loop result for the electron EDM and show that it bounds the imaginary part of the Higgs-electron coupling to be less than 1.7 x 10^-2 times the SM electron Yukawa coupling. Deviations of the real…

CouplingPhysicsParticle physicsNuclear and High Energy PhysicsLarge Hadron ColliderAnomalous magnetic dipole momentPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesElectron electric dipole momentStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonHigh Energy Physics::ExperimentJournal of High Energy Physics
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Improving Nearest Neighbor Based Multi-target Prediction Through Metric Learning

2017

The purpose of this work is to learn specific distance functions to be applied for multi-target regression problems using nearest neighbors. The idea of preserving the order relation between input and output vectors considering their corresponding distances is used along a maximal margin criterion to formulate a specific metric learning problem. Extensive experiments and the corresponding discussion try to put forward the advantages of the proposed algorithm that can be considered as a generalization of previously proposed approaches. Preliminary results suggest that this line of work can lead to very competitive algorithms with convenient properties.

Cover treeComputer scienceNearest neighbor search0211 other engineering and technologies02 engineering and technologyk-nearest neighbors algorithmBest bin firstMargin (machine learning)Nearest-neighbor chain algorithmMetric (mathematics)0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingAlgorithmLarge margin nearest neighbor021101 geological & geomatics engineering
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