Search results for "Spectral"

showing 10 items of 3116 documents

Spectral imaging system for money counterfeit detection

2019

A prototype with three different wavelength lasers (448nm, 532nm and 659nm) for money counterfeit illumination, analyzation and detection using RGB crosstalk correction and comparing spectral image ration for different banknote elements will be presented.

Physicsmedicine.medical_specialtybusiness.industryLaserCounterfeitSpectral imaginglaw.inventionCrosstalkWavelengthOpticslawSpectral imagemedicineRGB color modelImage sensorbusinessImaging and Applied Optics 2019 (COSI, IS, MATH, pcAOP)
researchProduct

Compressive single-pixel multispectral Stokes polarimeter

2014

We present a single-pixel system that performs polarimetric multispectral imaging with the aid of compressive sensing techniques. We experimentally obtain the full Stokes spatial distribution of a scene for different spectral channels.

Physicsmedicine.medical_specialtybusiness.industryMultispectral imageComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONPolarimetryHyperspectral imagingPolarimeterMultispectral pattern recognitionSpectral imagingComputer Science::GraphicsCompressed sensingOpticsComputer Science::Computer Vision and Pattern RecognitionFull spectral imagingComputer Science::MultimediamedicinebusinessPhysics::Atmospheric and Oceanic PhysicsComputingMethodologies_COMPUTERGRAPHICSRemote sensingLatin America Optics and Photonics Conference
researchProduct

Spectral imaging system for scaling the power spectrum of optical waveforms.

2007

We propose and analyze a new photonic system to change the scale of the optical power spectrum of an ultrashort pulse. Our device corresponds to the dual (spectral domain) configuration of a temporal imaging system. It is configured with two time lenses separated by a linear first-order dispersive medium. The specific relation between the chirp rates and the first-order dispersion coefficient is obtained. The main practical constraints are discussed, and the system performance is tested by means of a numerical simulation.

Physicsmedicine.medical_specialtybusiness.industryPhysics::OpticsSpectral densityOptical powerPulse shapingAtomic and Molecular Physics and OpticsSpectral imagingOpticsChirpmedicinePhotonicsbusinessUltrashort pulsePhotonic-crystal fiberOptics letters
researchProduct

2019

We demonstrate experimentally ghost optical coherence tomography using a broadband incoherent supercontinuum light source with shot-to-shot random spectral fluctuations. The technique is based on ghost imaging in the spectral domain where the object is the spectral interference pattern generated from an optical coherence tomography interferometer in which a physical sample is placed. The axial profile of the sample is obtained from the Fourier transform of the correlation between the spectrally resolved intensity fluctuations of the supercontinuum and the integrated signal measured at the output of the interferometer. The results are in excellent agreement with measurements obtained from a …

Physicsmedicine.medical_specialtymedicine.diagnostic_testbusiness.industryPhysics::Optics02 engineering and technologyGhost imaging021001 nanoscience & nanotechnology01 natural sciencesSignalAtomic and Molecular Physics and OpticsSupercontinuumSpectral imaging010309 opticssymbols.namesakeInterferometryOpticsFourier transformOptical coherence tomography0103 physical sciencesBroadbandmedicinesymbols0210 nano-technologybusinessOptics Express
researchProduct

X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391

2005

We present X-ray spectral and timing analysis of members of the young open cluster IC 2391 observed with the XMM-Newton observatory. We detected 99 X-ray sources by analysing the summed data obtained from MOS1, MOS2 and pn detectors of the EPIC camera; 24 of them are members, or probable members, of the cluster. Stars of all spectral types have been detected, from the early-types to the late-M dwarfs. Despite the capability of the instrument to recognize up to 3 thermal components, the X-ray spectra of the G, K and M members of the cluster are well described with two thermal components (at kT$_1 \sim$ 0.3-0.5 keV and kT$_2 \sim$ 1.0-1.2 keV respectively) while the X-ray spectra of F members…

Physicsopen clusters and associations : individual : IC 2391 OPEN CLUSTERSAstrophysics (astro-ph)X-rayFOS: Physical sciencesstars : late-typeAstronomy and AstrophysicsAstrophysicsX-ray : starAstrophysicsStellar classificationSpectral linePLEIADESstars : activityVARIABILITYStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceObservatoryROSATstars; stars : activity; stars : early-type; stars : late-type; open clusters and associations : individual : IC 2391 OPEN CLUSTERS; EMISSION; PLEIADES; VARIABILITY [X-ray]Cluster (physics)stars : early-typeEMISSIONOpen clusterAstronomy & Astrophysics
researchProduct

Shape from polarization: a method for solving zenithal angle ambiguity

2012

International audience; We report a multispectral based method that permits the evolution of shape from polarization setup applied to 3D shape estimation of transparent objects. The setup is based on a polarization imaging technique which is a recent imaging method based on the analysis of the polarization state of the light in the observed scene. The technique has rapidly evolved with the development of electro-optic components and some polarization cameras are now available on the market. Shape from polarization consists in measuring the azimuthal and zenithal angles characterizing the normal of each point of the observed surface. We focus on the ambiguity in the measurement of the zenith…

Physicspolarization imaging[SPI.OPTI] Engineering Sciences [physics]/Optics / Photonicbusiness.industrymedia_common.quotation_subject010401 analytical chemistryMultispectral imagePolarization imagingAmbiguityPolarization (waves)01 natural sciencesAtomic and Molecular Physics and Optics3D shape0104 chemical sciences010309 opticsAzimuthOpticsComputer Science::Computer Vision and Pattern Recognition0103 physical sciences[SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic[ SPI.OPTI ] Engineering Sciences [physics]/Optics / PhotonicbusinessRefractive indexmedia_common
researchProduct

Corrigendum: Spectral Entropy Based Neuronal Network Synchronization Analysis Based on Microelectrode Array Measurements

2020

Physicsrat cortical cellsSpectral entropyspectral entropyNeuroscience (miscellaneous)developing neuronal networksMultielectrode arraylcsh:RC321-571Cellular and Molecular NeurosciencecorrelationSynchronization (computer science)Biological neural networkmouse cortical cellsBiological systemsynchronizationlcsh:Neurosciences. Biological psychiatry. NeuropsychiatryFrontiers in Computational Neuroscience
researchProduct

Chandra observation of the Big Dipper X 1624–490

2006

We present the results of a 73 ks long Chandra observation of the dipping source X 1624-490. During the observation a complex dip lasting 4 hours is observed. We analyse the persistent emission detecting, for the first time in the 1st-order spectra of X 1624-490, an absorption line associated to \ion{Ca}{xx}. We confirm the presence of the \ion{Fe}{xxv} K$_\alpha$ and \ion{Fe}{xxvi} K$_\alpha$ absorption lines with a larger accuracy with respect to a previous XMM observation. Assuming that the line widths are due to a bulk motion or a turbulence associated to the coronal activity, we estimate that the lines have been produced in a photoionized absorber between the coronal radius and the out…

Physicsstars : individual : X 1624-490Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysicsaccretion accretion diskstars : neutronBulk motionSpectral lineIonAccretion discSpace and Planetary ScienceX-rays : starX-rays : binarieindividual : X 1624-490; stars : neutron; X-rays : stars; X-rays : binaries; X-rays : general [accretion accretion disks; stars]X-rays : generalLine (formation)Astronomy & Astrophysics
researchProduct

Relativistically Smeared Iron Lines in the Spectra of Bright NS LMXB

2009

We present preliminary results of a study on three bright accreting low-mass X-ray binaries hosting a neutron star, based on XMM-Newton observations. These sources (GX 340+0, GX 349+2 and SAX J1808.4-3658) show a broad Fe K alpha iron line in their spectra. This feature can be well described by relativistic line profile in each case; the good spectral resolution of the EPIC/PN and the high statistics spectra allow to put very good constraints on the disk geometry and ionization stage of the reflecting matter.

Physicsstars: neutron starAstrophysics::High Energy Astrophysical Phenomenastars: individual: GX 340+0 GX 349+2 SAX J1808.4-3658X-ray: starAstronomyAstrophysicsEPICX-ray: spectrumSpectral lineNeutron starSettore FIS/05 - Astronomia E Astrofisicaindividual: GX 340+0 GX 349+2 SAX J1808.4-3658; stars: neutron stars; X-ray: stars; X-ray: spectrum; [accretion disks; stars]PulsarIonizationSpectral resolutionSpectroscopyaccretion diskLine (formation)
researchProduct

The bound state in the spectrum of the Lee–Friedrichs Hamiltonian

2000

Abstract The spectrum of the Lee–Friedrichs Hamiltonian, describing a two-level system embedded in a continuum, is considered. An appropriate discretization of the field modes is performed before taking the continuum limit. It is shown that the existence of an eigenstate with negative energy (bound state) is related to the nonanalyticity of the Friedrichs spectral representation. This negative energy state is a dressed state and its physical properties are studied in some significant cases.

Physicssymbols.namesakeSpectral representationDiscretizationQuantum mechanicsBound statesymbolsGeneral Physics and AstronomyNegative energyHamiltonian (quantum mechanics)Eigenvalues and eigenvectorsPhysics Letters A
researchProduct