Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

2021

Abstract We propose a signal deconvolution procedure for imaging spectrometer data, where a measured point spread function (PSF) is deconvolved itself before being used for deconvolution of the signal. We evaluate the effectiveness of our procedure for improvement of the spatio-spectral signal, as well as our target application, i.e. estimation of sun-induced fluorescence (SIF). Imaging spectrometers are well established instruments for remote sensing. When used for scientific purposes these instruments are usually calibrated on a regular basis. In our case the point spread function of the optics is measured in an elaborate procedure with a tunable monochromator point light source. PSFs are…

Point spread functionmedicine.medical_specialtyComputer scienceWiener filterAstrophysics::Instrumentation and Methods for AstrophysicsImaging spectrometerSoil ScienceHyperspectral imagingGeologyPeak signal-to-noise ratioSpectral imagingsymbols.namesakesymbolsmedicineDeconvolutionComputers in Earth SciencesImage sensorAlgorithmRemote sensingRemote Sensing of Environment
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Linear infrared dichroism by a double modulation technique

1991

In the first part of this paper an experimental setup using Fourier-transform infrared spectroscopy (FTIR) in combination with a photoelastic modulator (PEM) for linear dichroism measurements is described. The second part shows the influence of PEM-amplitude and scan-velocity on the sensitivity of the instrument. The third part deals with the fringe-problem in the baselines of absorbance spectra and its influence on the determination of the linear dichroic ratio.

Polymers and PlasticsPhotoelastic modulatorInfrared dichroismbusiness.industryChemistryOrganic ChemistryAstrophysics::Instrumentation and Methods for AstrophysicsAnalytical chemistryPhysics::OpticsInfrared spectroscopyCondensed Matter PhysicsLinear dichroismDichroic glassOpticsModulationMaterials ChemistrySensitivity (control systems)Physics::Chemical PhysicsFourier transform infrared spectroscopybusinessMakromolekulare Chemie. Macromolecular Symposia
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Photo-z optimization for measurements of the BAO radial scale

2009

ArXiv pre-print avaible at:http://arxiv.org/abs/0812.3414

PopulationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicspower spectrumLambda01 natural sciencesComputer Science::Digital LibrariesSpectral lineComputer Science::Computational Engineering Finance and Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysicseducation.field_of_study010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsShot noiseAstronomy and Astrophysicssuveys of galaxiesRedshiftGalaxyAstronomiaAstrophysics::Earth and Planetary AstrophysicsBaryon acoustic oscillations
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The positioning system of the ANTARES Neutrino Telescope

2012

The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning sys…

Positioning systemDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Detector modelling and simulations II (electric fieldsDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesTiming detectorshardwareDetector alignment and calibration methods010303 astronomy & astrophysicsInstrumentationDETECTOR ALIGMENTMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSOUND[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Orientation (computer vision)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsTriangulation (computer vision)particle-beams)GeodesyDETECTOR CONTROL SYSTEMDetector modelling and simulations II (electric fields charge transport multiplication and induction pulse formation electron emission etc)Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)sources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pulse formationarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2DETECTOR MODELLING AND SIMULATIONSDetector modelling and simulations IIalgorithmsPhysics::Geophysics0103 physical sciences14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationetc)multiplication and inductionBuoyDetector control systems010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsMooringcharge transport[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Detector alignment and calibration methods (laserselectron emissionFISICA APLICADAdetector modelling and simulations ii (electric fields; antares neutrino telescope; multiplication and induction; charge transport; pulse formation; electron emission; etc); hardware; architecture; timing detectors; detector control systems (detector and experiment monitoring and slow-control systems; algorithms; databases); sources; detector alignment; calibration.; acoustic positioning; detector alignment and calibration methods (lasers; particle-beams)
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

2019

The determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it allows us to significantly reduce the systematic uncertainties related to the mass composition and th…

Primary energyAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesNuclear physicscosmic rays0103 physical sciencesExperiments in gravityddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGénéralitésDETETORESMODEL13. Climate actioncosmic rays detectors ultra high energy cosmic raysExperimental High Energy Physicscosmic rays detectorsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyEnergy (signal processing)Physical Review D
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Metabolic flux understanding of Pichia pastoris grown on heterogenous culture media

2014

[EN] Within the emergent field of Systems Biology, mathematical models obtained from physical chemical laws (the so-called first principles-based models) of microbial systems are employed to discern the principles that govern cellular behaviour and achieve a predictive understanding of cellular functions. The reliance on this biochemical knowledge has the drawback that some of the assumptions (specific kinetics of the reaction system, unknown dynamics and values of the model parameters) may not be valid for all the metabolic possible states of the network. In this uncertainty context, the combined use of fundamental knowledge and data measured in the fermentation that describe the behaviour…

Principal Component AnalysisbiologyMathematical modelManufacturing processComputer scienceProcess Chemistry and TechnologySystems biologyMonte Carlo samplingESTADISTICA E INVESTIGACION OPERATIVACellular functionsMetabolic networkMetabolic networkMissing-data methods for Exploratory Data AnalysisContext (language use)biology.organism_classificationINGENIERIA DE SISTEMAS Y AUTOMATICAComputer Science ApplicationsAnalytical ChemistryPichia pastorisEconometricsBiochemical engineeringPossibilistic consistency analysisFlux (metabolism)SpectroscopySoftware
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Characterization of the atmospheric muon flux in IceCube

2015

Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event yield in large-volume underground particle detectors. The IceCube detector, with an instrumented volume of about a cubic kilometer, has the potential to conduct unique investigations on atmospheric muons by exploiting the large collection area and the possibility to track particles over a long distance. Through detailed reconstruction of energy deposition along the tracks, the characteristics of muon bundles can be quantified, and individual particles of exceptionally high energy identified. The data can then be used to constrain the cosmic ray primary flux and the contribution to atmospheric …

Prompt leptonsleptonAtmospheric muons; Cosmic rays; Prompt leptons; Astronomy and AstrophysicsPhysics::Instrumentation and DetectorsHadronAtmospheric muonsprimary [cosmic radiation]PROTON01 natural sciencesIceCubesurface [detector]atmosphere [muon]NEUTRINO TELESCOPEproduction [muon]PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)ELEMENTAL GROUPSDetectormodel [interaction]Astrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAY MUONSENERGY-SPECTRUMvector mesonstatisticsINTRINSIC CHARMddc:540Physique des particules élémentaireshigh [energy]Astrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]Atmosperic muonsexceptionalairflux [muon]Astrophysics::High Energy Astrophysical Phenomenaspectrum [multiplicity]energy spectrumFOS: Physical sciencesCosmic rayatmosphere [cosmic radiation]Nuclear physicscosmic rays0103 physical sciencesARRIVAL DIRECTIONSVector meson010306 general physicsCosmic raysZenithANISOTROPYMuon010308 nuclear & particles physicsAstronomy and AstrophysicsSpectral componenttracksMODELPhysics and Astronomy13. Climate actionTEVspectralHigh Energy Physics::ExperimenthadronLepton
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Step-along power vector method for astigmatic wavefront propagation

2013

Purpose To propose both a new algebraic solution and a graphical monitoring method for astigmatic wavefront propagation in the framework provided by power vectors. Methods The generalised propagation equation describing the propagation of astigmatic wavefronts from one plane to another is adapted to the power vectors formalism using a novel algorithm based on a step-along method. The step-along procedure is directly applied to the tuple of power vectors [M, J0, J45] representing an arbitrary astigmatic wavefront and it permits the calculation of the tuple of power vectors [M′, J′0, J′45] after a given propagation distance. This is achieved mathematically first by temporarily rotating the as…

Propagation equationWavefrontOptics and PhotonicsLightAlgebraic solutionbusiness.industryMathematical analysisAstrophysics::Instrumentation and Methods for AstrophysicsAstigmatismPhysics::OpticsPower vectorSensory SystemsOphthalmologyEyeglassesOpticsHomogeneousHumansMonitoring methodsAlgebraic numberTuplebusinessMathematicsOptometryMathematicsOphthalmic and Physiological Optics
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Virtual and arrow Temperley–Lieb algebras, Markov traces, and virtual link invariants

2021

Let [Formula: see text] be the algebra of Laurent polynomials in the variable [Formula: see text] and let [Formula: see text] be the algebra of Laurent polynomials in the variable [Formula: see text] and standard polynomials in the variables [Formula: see text] For [Formula: see text] we denote by [Formula: see text] the virtual braid group on [Formula: see text] strands. We define two towers of algebras [Formula: see text] and [Formula: see text] in terms of diagrams. For each [Formula: see text] we determine presentations for both, [Formula: see text] and [Formula: see text]. We determine sequences of homomorphisms [Formula: see text] and [Formula: see text], we determine Markov traces […

Pure mathematicsAlgebra and Number TheoryMarkov chainComputer Science::Information Retrieval010102 general mathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)0102 computer and information sciences01 natural sciencesTheoryofComputation_MATHEMATICALLOGICANDFORMALLANGUAGES010201 computation theory & mathematicsComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGArrowComputer Science::General Literature0101 mathematicsAlgebra over a fieldVirtual linkComputingMilieux_MISCELLANEOUSMathematicsVariable (mathematics)Journal of Knot Theory and Its Ramifications
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Manifolds and Smooth Mappings

2020

This is a preparatory chapter giving the necessary standard background on smooth and complex manifolds and maps.

Pure mathematicsAstrophysics::Instrumentation and Methods for AstrophysicsMathematics::Differential GeometryMathematics::Symplectic GeometryMathematics
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