Search results for "Correlation function"

showing 4 items of 164 documents

The ALHAMBRA survey: evolution of galaxy clustering since z∼1

2014

We study the clustering of galaxies as function of luminosity and redshift in the range $0.35 < z < 1.25$ using data from the Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) survey. The ALHAMBRA data used in this work cover $2.38 \mathrm{deg}^2$ in 7 independent fields, after applying a detailed angular selection mask, with accurate photometric redshifts, $��_z \lesssim 0.014 (1+z)$, down to $I_{\rm AB} < 24$. Given the depth of the survey, we select samples in $B$-band luminosity down to $L^{\rm th} \simeq 0.16 L^{*}$ at $z = 0.9$. We measure the real-space clustering using the projected correlation function, accounting for photometric redshifts uncert…

statistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCorrelation function (astronomy)01 natural sciencesPhysical cosmologyLuminosityLarge-scale structure of Universe.0103 physical sciencesRange (statistics)distances and redshifts [Galaxies]Sample variance10. No inequalitydata analysis [Methods]observations [Cosmology]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsGalaxyRedshiftSpace and Planetary ScienceHaloAstrophysics - Cosmology and Nongalactic Astrophysics
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Measuring galaxy segregation with the mark connection function

2010

(abridged) The clustering properties of galaxies belonging to different luminosity ranges or having different morphological types are different. These characteristics or `marks' permit to understand the galaxy catalogs that carry all this information as realizations of marked point processes. Many attempts have been presented to quantify the dependence of the clustering of galaxies on their inner properties. The present paper summarizes methods on spatial marked statistics used in cosmology to disentangle luminosity, colour or morphological segregation and introduces a new one in this context, the mark connection function. The methods used here are the partial correlation functions, includi…

statistical [Methods]Spatial correlationCosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of UniversePopulationFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCorrelation function (astronomy)UNESCO::ASTRONOMÍA Y ASTROFÍSICAUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasdata analysis [Methods]educationCluster analysisPartial correlationPhysicseducation.field_of_studyAstronomy and AstrophysicsFunction (mathematics)GalaxyLarge-scale structure of Universe; Methods : data analysis; Methods : statisticalSpace and Planetary Science:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]Astrophysics - Cosmology and Nongalactic Astrophysics
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Scattering of Co-Current Surface Waves on an Analogue Black Hole

2018

We report on what is to our knowledge the first scattering experiment of surface waves on an accelerating transcritical flow, which in the analogue gravity context is described by an effective spacetime with a black-hole horizon. This spacetime has been probed by an incident co-current wave, which partially scatters into an outgoing countercurrent wave on each side of the horizon. The measured scattering amplitudes are compatible with the predictions of the hydrodynamical theory, where the kinematical description in terms of the effective metric is exact.

surface: deformationGeneral Physics and AstronomyFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)black hole: horizonGravitation and Astrophysics01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceswave: scatteringsurfaceeffect: Hawkingcorrelation function010306 general physicsPhysicsSpacetimeScatteringHorizonFluid Dynamics (physics.flu-dyn)Physics - Fluid Dynamics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Scattering amplitudeBlack holeFlow (mathematics)space-timeSurface waveQuantum electrodynamics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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Two-particle transverse momentum correlations in pp and p-Pb collisions at energies available at the CERN Large Hadron Collider

2023

Two-particle transverse momentum differential correlators, recently measured in Pb--Pb collisions at energies available at the CERN Large Hadron Collider (LHC), provide an additional tool to gain insights into particle production mechanisms and infer transport properties, such as the ratio of shear viscosity to entropy density, of the medium created in Pb-Pb collisions. The longitudinal long-range correlations and the large azimuthal anisotropy measured at low transverse momenta in small collision systems, namely pp and p-Pb, at LHC energies resemble manifestations of collective behaviour. This suggests that locally equilibrated matter may be produced in these small collision systems, simil…

two particle correlations large hadron colliderCERN Lablongitudinallarge hadron colliderheavy ion scatteringcollectiveFOS: Physical sciencesanisotropy measuredtransverse momentum correlation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)transport theoryTeVcorrelation functionNuclear Experiment (nucl-ex)Nuclear ExperimentMonte Carloeffect viscositycorrelation long-rangetwo-particleentropy densityparticle multiplicityCERN LHC Collangular distribution anisotropybroadeningtransverse momentum lowydinfysiikkatwo particle correlations
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