Search results for "Number density"

showing 10 items of 19 documents

ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test case

2017

We present ELDAR, a new method that exploits the potential of medium- and narrow-band filter surveys to securely identify active galactic nuclei (AGN) and determine their redshifts. Our methodology improves on traditional approaches by looking for AGN emission lines expected to be identified against the continuum, thanks to the width of the filters. To assess its performance, we apply ELDAR to the data of the ALHAMBRA (Advance Large Homogeneous Area Medium Band Redshift Astronomical) survey, which covered an effective area of 2.38 deg2 with 20 contiguous medium-band optical filters down to F814W ≃ 24.5. Using two different configurations of  ELDAR in which we require the detection of at lea…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies][ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Continuum (design consultancy)FOS: Physical sciencesAstrophysicsSurveys01 natural sciencestechniques: photometricemission lines [Quasars]Galaxies: distances and redshiftssurveys0103 physical sciencesdistances and redshifts [Galaxies]Emission spectrumOptical filterdata analysis [Methods]010303 astronomy & astrophysicsPhysicsANÁLISE DE DADOSNumber density010308 nuclear & particles physicsphotometric [Techniques]galaxies: active – galaxies: distances and redshiftsAstronomy and AstrophysicsFilter (signal processing)Galaxies: activeAstrophysics - Astrophysics of Galaxiesmethods: data analysisGalaxyRedshiftquasars: emission linesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Modelling accretion disc and stellar wind interactions: the case of Sgr A*

2016

Sgr A* is an ideal target to study low-luminosity accreting systems. It has been recently proposed that properties of the accretion flow around Sgr A* can be probed through its interactions with the stellar wind of nearby massive stars belonging to the S-cluster. When a star intercepts the accretion disk, the ram and thermal pressures of the disk terminate the stellar wind leading to the formation of a bow shock structure. Here, a semi-analytical model is constructed which describes the geometry of the termination shock formed in the wind. With the employment of numerical hydrodynamic simulations, this model is both verified and extended to a region prone to Kelvin-Helmholtz instabilities. …

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural scienceslaw.inventionGravitationlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSupermassive black holeNumber densityBremsstrahlungAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Stars13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaHeliosphereFlareMonthly Notices of the Royal Astronomical Society
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Enhanced crystal stability in a binary mixture of charged colloidal spheres.

2009

We report on the phase behavior of a binary charged sphere mixture of size ratio $\ensuremath{\Gamma}=0.68$ and charge ratio $\ensuremath{\Lambda}\ensuremath{\approx}1$ as a function of composition $p$ and number density $n$. For $p=0.1--0.3$ we observe freezing at densities well below the freezing densities of the pure components. At all compositions our data indicate the formation of substitutional alloy crystals of body centered cubic structure. No indications for compound formation were observed. Rather, our findings point at the first observation of an upper azeotrope. Measurements of the crystallization kinetics reveal a combined density and composition dependence of growth velocities…

CrystalColloidNumber densityMaterials scienceAzeotropePhase (matter)NucleationThermodynamicsCharge (physics)Cubic crystal systemPhysical review. E, Statistical, nonlinear, and soft matter physics
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NGC1600 - Cluster or Field Elliptical?

2008

A study of the galaxy distribution in the field of the elliptical galaxy NGC1600 has been undertaken. Although this galaxy is often classified as a member of a loose group, all the neighbouring galaxies are much fainter and could be taken as satellites of NGC1600. The number density profile of galaxies in the field of this galaxy shows a decline with radius, with evidence of a background at approximately 1.3 Mpc. The density and number density profile are consistent with that found for other isolated early-type galaxies. NGC1600 appears as an extended source in X-rays, and the center of the X-ray emission seems not to coincide with the center of the galaxy. The velocity distribution of neig…

PhysicsSolar massNumber densityField (physics)Astrophysics (astro-ph)Velocity dispersionFOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxyRadial velocitySpace and Planetary ScienceElliptical galaxyAstrophysics::Galaxy Astrophysics
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The role of connectivity in the properties of sedimented materials

2003

Effective-medium theories for both random packings of elastic discs and mats of randomly sedimented elastic fibers can be constructed such that the effective material stiffness depends on the stiffness and geometry of the constituents of the material, and the number density of contacts. It is demonstrated that the number density of contacts together with the geometry of the constituents also determine the porosity of these materials. The simplicity and similar structure of the effective-medium estimates for the properties of these two qualitatively different materials indicate that the number density of contacts may play a similar role in an appropriate effective-medium description of a lar…

Large classNumber densityMaterials scienceMechanics of MaterialsmedicineGeneral Physics and AstronomyDeposition (phase transition)StiffnessGeneral Materials ScienceComposite materialmedicine.symptomElasticity (economics)PorosityGranular Matter
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High-Yield Growth and Tunable Morphology of Bi2Se3 Nanoribbons Synthesized on Thermally Dewetted Au

2021

The yield and morphology (length, width, thickness) of stoichiometric Bi2Se3 nanoribbons grown by physical vapor deposition is studied as a function of the diameters and areal number density of the Au catalyst nanoparticles of mean diameters 8–150 nm formed by dewetting Au layers of thicknesses 1.5–16 nm. The highest yield of the Bi2Se3 nanoribbons is reached when synthesized on dewetted 3 nm thick Au layer (mean diameter of Au nanoparticles ~10 nm) and exceeds the nanoribbon yield obtained in catalyst-free synthesis by almost 50 times. The mean lengths and thicknesses of the Bi2Se3 nanoribbons are directly proportional to the mean diameters of Au catalyst nanoparticles. In contrast, the me…

Materials scienceNumber densityYield (engineering)synthesisGeneral Chemical EngineeringAnalytical chemistryNanoparticleBi<sub>2</sub>Se<sub>3</sub>ChemistryPhysical vapor depositionnanoribbonGeneral Materials ScienceDewettingQD1-999physical vapor depositionNanoscopic scaleStoichiometryDeposition (law)Nanomaterials
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Joint constraints on galaxy bias and σ8 through the N-pdf of the galaxy number density

2015

We present a full description of the N-probability density function of the galaxy number density fluctuations. This N-pdf is given in terms, on the one hand, of the cold dark matter correlations and, on the other hand, of the galaxy bias parameter. The method relies on the assumption commonly adopted that the dark matter density fluctuations follow a local non-linear transformation of the initial energy density perturbations. The N-pdf of the galaxy number density fluctuations allows for an optimal estimation of the bias parameter (e.g., via maximum-likelihood estimation, or Bayesian inference if there exists any a priori information on the bias parameter), and of those parameters defining …

PhysicsNumber densityCold dark matter010308 nuclear & particles physicsModel selectionDark matterEstimatorAstronomy and AstrophysicsProbability density functionAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy0103 physical sciencesStatistical physics010303 astronomy & astrophysicsGalaxy clusterAstrophysics - Cosmology and Nongalactic Astrophysics
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Observational Results On The Influence Of Surface Layer Stability And Inversion Entrainment On Surface Layer Marine Aerosol Number Density (1 Microme…

1983

Wind speed and relative humidity have been the physical variables used in empirical expressions for equilibrium marine aerosol distributions. Recent formulations, which include the role of hydrostatic stability because it influences turbulent transport and entrainment of clear air from aloft, are examined on the basis of 1 um radius aerosol number density values. The aerosol data were collected along with a quite complete meteorological data set in the Northeast Atlantic during the international Joint Air Sea Interaction Experiment (JASIN-78). The 1 um number density values are normalized for generation and relative humidity influences, and analyses are performed to gain reasonable assuranc…

food.ingredientNumber densitySea saltGeneral EngineeringHumidityAtmospheric sciencesAtomic and Molecular Physics and Opticslaw.inventionAerosolBoundary layerfoodlawEnvironmental scienceRelative humiditySurface layerHydrostatic equilibriumOptical Engineering
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Rubidium dimers in paraffin-coated cells

2010

Measurements were made to determine the density of rubidium dimer vapor in paraffin-coated cells. The number density of dimers and atoms in similar paraffin-coated and uncoated cells was measured by optical spectroscopy. Due to the relatively low melting point of paraffin, a limited temperature range of 43-80 deg C was explored, with the lower end corresponding to a dimer density of less than 10^7 cm^(-3). With one-minute integration time, a sensitivity to dimer number density of better than 10^6 cm^(-3) was achieved. No significant difference in dimer density was observed between the cells.

Time delay and integrationPhysicsQuantum PhysicsNumber densityAtomic Physics (physics.atom-ph)DimerSignificant differenceAnalytical chemistryGeneral Physics and Astronomychemistry.chemical_elementLow melting pointFOS: Physical sciences02 engineering and technologyAtmospheric temperature range021001 nanoscience & nanotechnology01 natural sciencesPhysics - Atomic PhysicsRubidiumchemistry.chemical_compoundchemistry0103 physical sciences010306 general physics0210 nano-technologySpectroscopyQuantum Physics (quant-ph)
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Observation of laser-induced field-free permanent planar alignment of molecules

2011

International audience; Permanent planar alignment of gas-phase linear molecules is achieved by a pair of delayed perpendicularly polarized short laser pulses. The experiment is performed in a supersonic jet, ensuring a relatively high number density of molecules with moderately low rotational temperature. The effect is optically probed on a femtosecond time scale by the use of a third short pulse, enabling a time-resolved birefringence detection performed successively in two perpendicular planes of the laboratory frame. The technique allows for an unambiguous estimation of the molecular planar delocalization produced within the polarization plane of the pulse pair after the turn-off of the…

[ PHYS.PHYS.PHYS-ATOM-PH ] Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Linear molecular geometry01 natural sciencesMolecular physicslaw.invention010309 opticsRotational dynamicsPlanarOpticslaw0103 physical sciencesUltrafast nonlinear optics010306 general physicsOptical Kerr effectPhysicsNumber densityBirefringence[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Molecular alignmentbusiness.industryFemtosecond phenomenaRotational temperature3710Vz 4250Hz 4250MdLaserPolarization (waves)Atomic and Molecular Physics and OpticsOptical polarigraphyFemtosecondbusiness
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