Search results for "Computer Vision"

showing 10 items of 2353 documents

Measuring Spatiotemporal Dependencies in Bivariate Temporal Random Sets with Applications to Cell Biology

2008

Analyzing spatiotemporal dependencies between different types of events is highly relevant to many biological phenomena (e.g., signaling and trafficking), especially as advances in probes and microscopy have facilitated the imaging of dynamic processes in living cells. For many types of events, the segmented areas can overlap spatially and temporally, forming random clumps. In this paper, we model the binary image sequences of two different event types as a realization of a bivariate temporal random set and propose a nonparametric approach to quantify spatial and spatiotemporal interrelations using the pair correlation, cross-covariance, and the Ripley K functions. Based on these summary st…

Covariance functionModels BiologicalSensitivity and SpecificityPattern Recognition Automated03 medical and health sciences0302 clinical medicineArtificial IntelligenceImage Interpretation Computer-AssistedCells CulturedIndependence (probability theory)030304 developmental biologyMathematics0303 health sciencesModels Statisticalbusiness.industryStochastic processApplied MathematicsNonparametric statisticsReproducibility of ResultsEstimatorImage EnhancementEndocytosisTemporal databaseMicroscopy FluorescenceComputational Theory and Mathematics[SDV.NEU]Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC]Computer Vision and Pattern RecognitionArtificial intelligenceCross-covariancebusinessAlgorithms030217 neurology & neurosurgerySoftwareRealization (probability)IEEE Transactions on Pattern Analysis and Machine Intelligence
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Vector anisotropic filter for multispectral image denoising

2015

In this paper, we propose an approach to extend the application of anisotropic Gaussian filtering for multi- spectral image denoising. We study the case of images corrupted with additive Gaussian noise and use sparse matrix transform for noise covariance matrix estimation. Specifically we show that if an image has a low local variability, we can make the assumption that in the noisy image, the local variability originates from the noise variance only. We apply the proposed approach for the denoising of multispectral images corrupted by noise and compare the proposed method with some existing methods. Results demonstrate an improvement in the denoising performance.

Covariance matrixbusiness.industryNoise reductionMultispectral imageComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONPattern recognitionNon-local meansNoisesymbols.namesakeGaussian noiseComputer Science::Computer Vision and Pattern RecognitionsymbolsComputer visionVideo denoisingArtificial intelligencebusinessMathematicsAnisotropic filteringTwelfth International Conference on Quality Control by Artificial Vision 2015
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Linear transform for simultaneous diagonalization of covariance and perceptual metric matrix in image coding

2003

Two types ofredundancies are contained in images: statistical redundancy and psychovisual redundancy. Image representation techniques for image coding should remove both redundancies in order to obtain good results. In order to establish an appropriate representation, the standard approach to transform coding only considers the statistical redundancy, whereas the psychovisual factors are introduced after the selection ofthe representation as a simple scalar weighting in the transform domain. In this work, we take into account the psychovisual factors in the de8nition of the representation together with the statistical factors, by means of the perceptual metric and the covariance matrix, res…

Covariance matrixbusiness.industryPattern recognitionCovarianceWeightingMatrix (mathematics)Redundancy (information theory)Artificial IntelligenceSignal ProcessingDiscrete cosine transformComputer Vision and Pattern RecognitionArtificial intelligencebusinessSoftwareTransform codingMathematicsImage compressionPattern Recognition
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Attitude estimation from polarimetric cameras

2018

International audience; In the robotic field, navigation and path planning applications benefit from a wide range of visual systems (e.g. perspective cameras, depth cameras, catadioptric cameras, etc.). In outdoor conditions, these systems capture information in which sky regions cover a major segment of the images acquired. However, sky regions are discarded and are not considered as visual cue in vision applications. In this paper, we propose to estimate attitude of Unmanned Aerial Vehicle (UAV) from sky information using a polarimetric camera. Theoretically , we provide a framework estimating the attitude from the skylight polarized patterns. We showcase this formulation on both simulate…

Cover (telecommunications)Computer sciencebusiness.industrymedia_common.quotation_subject020208 electrical & electronic engineeringPerspective (graphical)PolarimetryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION02 engineering and technologySkylightField (computer science)[SPI.AUTO]Engineering Sciences [physics]/AutomaticCatadioptric system[SPI.AUTO] Engineering Sciences [physics]/AutomaticSky0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingComputer visionArtificial intelligenceMotion planningbusiness[SPI.SIGNAL]Engineering Sciences [physics]/Signal and Image processingmedia_common[SPI.SIGNAL] Engineering Sciences [physics]/Signal and Image processing
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The TES-based cryogenic anticoincidence detector for IXO: First results from large area prototypes

2010

The technique which combines high resolution spectroscopy with imaging capability is a powerful tool to extract fundamental information in X-ray Astrophysics and Cosmology. TES (Transition Edge Sensors)-based microcalorimeters match at best the requirements for doing fine spectroscopy and imaging of both bright (high count rate) and faint (poor signal-to-noise ratio) sources. For this reason they are considered among the most promising detectors for the next high energy space missions and are being developed for use on the focal plane of the IXO (International X-ray Observatory) mission. In order to achieve the required signal-to-noise ratio for faint or diffuse sources it is necessary to r…

Cryogenic Detectors; IXO; SQUID; TES; X-ray; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringCryogenic DetectorsSQUIDSpace explorationX-raySignal-to-noise ratioOpticsSettore FIS/05 - Astronomia E AstrofisicaObservatoryElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringPhysicsSpectrometerPixelbusiness.industryApplied MathematicsDetectorPulse durationComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCardinal pointIXObusinessTES Cryogenic Detectors X-ray SQUID IXOTES
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Baseline design of the thermal blocking filters for the X-IFU detector on board ATHENA

2014

ATHENA is an advanced X-ray observatory designed by a large European consortium to address the science theme "Hot and Energetic Universe" recently selected by ESA for L2 – the second Large-class mission within the Cosmic Vision science program (launch scheduled in 2028). One of the key instruments of the mission is the X-ray Integral Field Unit (X-IFU), an array of Transition Edge Sensor (TES) micro-calorimeters with high energy resolution (2.5 eV @ 6 keV) in the energy range 0.2÷12 keV, operating at the focal plane of a large effective area high angular resolution (5" HEW) grazing incidence X-ray telescope. The X-IFU operates at temperatures below 100 mK and thus requires a sophisticated c…

CryostatCosmic VisionVisionShieldsX-ray telescopeGrazing incidencelaw.inventionTelescopeOpticsSettore FIS/05 - Astronomia E AstrofisicalawX-raysElectronicmicro-calorimeterOptical and Magnetic MaterialsElectrical and Electronic EngineeringX-ray telescopesPhysicsX-IFUSpatial resolutionSounding rocketEquipment and servicesbusiness.industrySensorsApplied MathematicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsOptical Blocking FiltersComputer Science Applications1707 Computer Vision and Pattern RecognitionDetector arraysCondensed Matter PhysicsATHENAmissionsCultural heritageTransition edge sensorbusinessATHENA; micro-calorimeter; missions; Optical Blocking Filters; X-IFU; X-rays; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringTelescopes
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Thermal modelling of the ATHENA X-IFU filters

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-IFU instrument of the ATHENA mission requires a set of thermal filters to reduce the photon shot noise onto its cryogenic detector and to protect it from molecular contamination. A set of five filters, operating at different nominal temperatures corresponding to the cryostat shield temperatures, is currently baselined. The knowledge of the actual filter temperature profi…

CryostatMaterials scienceCondensed Matter Physic01 natural sciencesthermal simulationSettore FIS/05 - Astronomia E AstrofisicaOpticsthermal filter0103 physical sciencesThermalEmissivityRadiative transferElectrical and Electronic Engineering010306 general physicsThermal analysis010303 astronomy & astrophysicsX-IFUbusiness.industryElectronic Optical and Magnetic MaterialDetectorShot noiseComputer Science Applications1707 Computer Vision and Pattern RecognitionATHENAApplied MathematicFilter (video)businessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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Radio frequency shielding of thin aluminized plastic filters investigated for the ATHENA X-IFU detector

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-ray Integral Field Unit (X-IFU) is one of the two detectors of the ATHENA astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensors (TES) micro-calorimeters covering a field of view of 5' diameter, sensitive in the energy range 0.2-12 keV, and providing a spectral resolution…

CryostatMaterials sciencePhysics::Instrumentation and DetectorsX-ray detectorRF attenuationField of viewCondensed Matter Physic02 engineering and technologyreverberation chamber7. Clean energyElectromagnetic interferenceSettore FIS/05 - Astronomia E AstrofisicaOpticsX-ray Integral Field Unit (X-IFU)thermal thin-film filter0202 electrical engineering electronic engineering information engineeringElectrical and Electronic Engineeringbusiness.industryElectronic Optical and Magnetic Material020502 materialsDetectorAstrophysics::Instrumentation and Methods for Astrophysicsx-ray detectorComputer Science Applications1707 Computer Vision and Pattern Recognition020206 networking & telecommunicationsresonance modeApplied MathematicATHENA X-ray observatoryEMI shielding0205 materials engineeringElectromagnetic shieldingRadio frequencyAntenna (radio)businessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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The focal plane assembly for the Athena X-ray Integral Field Unit instrument

2016

This paper summarizes a preliminary design concept for the focal plane assembly of the X-ray Integral Field Unit on the Athena spacecraft, an imaging microcalorimeter that will enable high spectral resolution imaging and point-source spectroscopy. The instrument's sensor array will be a ~ 3840-pixel transition edge sensor (TES) microcalorimeter array, with a frequency domain multiplexed SQUID readout system allowing this large-format sensor array to be operated within the thermal constraints of the instrument's cryogenic system. A second TES detector will be operated in close proximity to the sensor array to detect cosmic rays and secondary particles passing through the sensor array for off…

CryostatPhysics::Instrumentation and DetectorsAperture01 natural sciencesfrequency division multiplexingfocal plane assemblySettore FIS/05 - Astronomia E AstrofisicaOpticsSensor array0103 physical sciencesElectronicSQUID amplifierAthenaOptical and Magnetic MaterialsElectrical and Electronic Engineeringta216010306 general physicsta113010302 applied physicsPhysicsX-IFUta114ta213business.industryStray lightApplied Mathematicstransition edge sensorDetectorAstrophysics::Instrumentation and Methods for AstrophysicsX-ray microcalorimeterComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCardinal pointElectromagnetic shieldingcryogenic anti-coincidence detectorX-ray microcalorimeter transition edge sensor cryogenic anti-coincidence detector SQUID amplifier frequency division multiplexing Athena X-IFU focal plane assemblyTransition edge sensorbusinessAthena; cryogenic anti-coincidence detector; focal plane assembly; frequency division multiplexing; SQUID amplifier; transition edge sensor; X-IFU; X-ray microcalorimeter; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSPIE Proceedings
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Cover Feature: Electrochemical Installation of CFH 2 −, CF 2 H−, CF 3 −, and Perfluoroalkyl Groups into Small Organic Molecules (Chem. Rec. 9/2021)

2021

CrystallographyChemistryFeature (computer vision)General Chemical EngineeringMaterials ChemistryCover (algebra)General ChemistryElectrochemistryBiochemistryOrganic moleculesThe Chemical Record
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