Search results for "Cluster Analysis"

showing 10 items of 848 documents

Recovering the real-space correlation function from photometric redshift surveys

2008

Measurements of clustering in large-scale imaging surveys that make use of photometric redshifts depend on the uncertainties in the redshift determination. We have used light-cone simulations to show how the deprojection method successfully recovers the real space correlation function when applied to mock photometric redshift surveys. We study how the errors in the redshift determination affect the quality of the recovered two-point correlation function. Considering the expected errors associated to the planned photometric redshift surveys, we conclude that this method provides information on the clustering of matter useful for the estimation of cosmological parameters that depend on the la…

PhysicsAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsScale (descriptive set theory)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCorrelation function (astronomy)Space (mathematics)AstrophysicsGalaxyRedshiftDistribution (mathematics)Space and Planetary ScienceCluster analysisPhotometric redshift
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Elementary triangles in a 2D binary colloidal glass former

2005

Particle positions of a two-dimensional (2D) binary colloidal glass former were measured video-microscopically. Local density-optimized structures of triangles of nearest-neighboring particles (TNNP) were found from the shortest pair-distances. These are referred to as elementary triangles (ET)—exactly one for each 3-particle combination of the two kinds of colloids. Clustering of ET-like TNNP implies larger distances between two particles, which generate the near-zone maxima in the pair-distribution functions. Tiling mismatches of different kinds of ET create structural frustrations. Increasing combination possibilities for the tiling of the different ET lead to the loss of long-range orde…

PhysicsColloidmedia_common.quotation_subjectGeneral Physics and AstronomyFrustrationOrder (group theory)Binary numberParticleStatistical physicsMaximaCluster analysismedia_commonEurophysics Letters (EPL)
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Fractal Aspects of Galaxy Clustering

2008

In the past decade, the mathematical concept of fractal has exerted a great influence in a large variety of scientific disciplines. It is very common to find recent papers on the application of fractals to different fields in Physics, Chemistry, Biology, etc. The success of the fractal geometry in the description of many systems is due to the fact that deep insights into very simple objects show how fractal measures are more natural for their study.

PhysicsCorrelation dimensionFractalHausdorff dimensionAstronomyStatistical physicsCluster analysisFractal dimensionGalaxyVariety (cybernetics)Simple (philosophy)
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Searching for the scale of homogeneity

1998

We introduce a statistical quantity, known as the $K$ function, related to the integral of the two--point correlation function. It gives us straightforward information about the scale where clustering dominates and the scale at which homogeneity is reached. We evaluate the correlation dimension, $D_2$, as the local slope of the log--log plot of the $K$ function. We apply this statistic to several stochastic point fields, to three numerical simulations describing the distribution of clusters and finally to real galaxy redshift surveys. Four different galaxy catalogues have been analysed using this technique: the Center for Astrophysics I, the Perseus--Pisces redshift surveys (these two lying…

PhysicsCorrelation dimensionHomogeneity (statistics)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxyRedshiftFractalSpace and Planetary ScienceCluster (physics)Statistical physicsCluster analysisStatisticAstrophysics::Galaxy Astrophysics
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Exponents of non-linear clustering in scale-free one-dimensional cosmological simulations

2012

One dimensional versions of cosmological N-body simulations have been shown to share many qualitative behaviours of the three dimensional problem. They can resolve a large range of time and length scales, and admit exact numerical integration. We use such models to study how non-linear clustering depends on initial conditions and cosmology. More specifically, we consider a family of models which, like the 3D EdS model, lead for power-law initial conditions to self-similar clustering characterized in the strongly non-linear regime by power-law behaviour of the two point correlation function. We study how the corresponding exponent \gamma depends on the initial conditions, characterized by th…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSpectral densityAstronomy and AstrophysicsCosmologyNumerical integrationMetric expansion of spaceUniversality (dynamical systems)Nonlinear systemTheoretical physicsSpace and Planetary ScienceExponentStatistical physicsCluster analysisAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Multiscaling Properties of Large-Scale Structure in the Universe

1995

The large-scale distribution of galaxies and galaxy clusters in the universe can be described in the mathematical language of multifractal sets. A particularly significant aspect of this description is that it furnishes a natural explanation for the observed differences in clustering properties of objects of different density in terms of multiscaling, the generic consequence of the application of a local density threshold to a multifractal set. The multiscaling hypothesis suggests ways of improving upon the traditional statistical measures of clustering pattern (correlation functions) and exploring further the connection between clustering pattern and dynamics.

PhysicsMultidisciplinarygalaxieMultifractal systemGalaxyCosmologyConnection (mathematics)CosmologySet (abstract data type)Distribution (mathematics)statisticsCosmology; galaxies; large-scale structure of the universe; statisticsgalaxiesStatistical physicslarge-scale structure of the universeCluster analysisGalaxy cluster
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The Deterministic Annealing Filter: A new clustering method for gamma-ray tracking algorithms

2010

A new method of clustering for forward-tracking algorithms has been developed to reconstruct the tracks of gamma-rays in high-resolution detector systems such as AGATA (Advanced GAmma Tracking Array). This technique, called Deterministic Annealing Filter (DAF), comes from statistical physics and is used in high-energy physics. After a description of the DAF method and of the forward-tracking algorithm, the performance of this clustering method is discussed in terms of photopeak efficiency and peak-to-total ratio obtained with GEANT4 simulations for the AGATA geometry. A comparison with the standard so-called "cone clustering method" shows similar performances with a better photopeak efficie…

PhysicsNuclear and High Energy PhysicsGRETA010308 nuclear & particles physicsDetectorHigh multiplicityDeterministic annealingDeterministic annealing filter[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Tracking (particle physics)01 natural sciencesGERMANIUMBACKTRACKINGgamma-ray spectroscopyFilter (video)0103 physical sciencesDETECTORSAGATAgamma-ray trackingSPECTROMETER010306 general physicsCluster analysisInstrumentationAlgorithm
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Improvement of cosmological neutrino mass bounds

2016

The most recent measurements of the temperature and low-multipole polarization anisotropies of the cosmic microwave background from the Planck satellite, when combined with galaxy clustering data f ...

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsCosmic microwave backgroundAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsPolarization (waves)01 natural sciencesGalaxysymbols.namesake0103 physical sciencessymbolsNeutrinoPlanckAnisotropyCluster analysis010303 astronomy & astrophysicsHubble's lawPhysical Review D
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“Study of Pulsar Light Curves by Cluster Analysis”

1986

The distribution of the phase numbers, corresponding to the arrival times of the gamma-ray photons detected by the COS-B satellite from the directions of the Crab and Vela pulsars, is analyzed by a clustering technique with the aim to detect possible microstructures in the pulsed emission. The method is found to be promising especially in view of the future gamma-ray experiments where better photon counting statistics is expected.

PhysicsPhotonPulsarAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)SatelliteAstrophysicsVelaLight curveCluster analysisPhoton counting
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Clustering in non-self-conjugate nuclei

2012

PhysicsPhysics and Astronomy (miscellaneous)Statistical physicsCluster analysisConjugate
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