Search results for "LIGHT"

showing 10 items of 3575 documents

Midinfrared FT-IR as a Tool for Monitoring Herbaceous Biomass Composition and Its Conversion to Furfural

2015

A semiquantitative analysis by means of midinfrared FT-IR spectroscopy was tuned for the simultaneous determination of cellulose, hemicellulose, and lignin in industrial crops such as giant reed (Arundo donaxL.) and switchgrass (Panicum virgatumL.). Ternary mixtures of pure cellulose, hemicellulose, and lignin were prepared and a direct correlation area/concentration was achieved for cellulose and lignin, whereas indirect correlations were found for hemicellulose quantification. Good correspondences between the values derived from our model and those reported in the literature or obtained according to the official Van Soest method were ascertained. Average contents of 40–45% of cellulose, 2…

Article SubjectbiologySpectroscopy; Analytical Chemistry; Atomic and Molecular Physics and OpticsArundo donaxSettore ING-IND/27 - Chimica Industriale E Tecnologicabiology.organism_classificationFurfuralAtomic and Molecular Physics and OpticsAnalytical Chemistrychemistry.chemical_compoundHydrolysischemistryAtomic and Molecular PhysicsYield (chemistry)Biomass characterization FTIR lignocellulose biomass pretreatmentlcsh:QC350-467Panicum virgatumLigninOrganic chemistryHemicelluloseand OpticsCelluloselcsh:Optics. LightSpectroscopyNuclear chemistryJournal of Spectroscopy
researchProduct

Study of ambient light influence for three-dimensional scanners based on structured light

2007

Ambient light in a scene can introduce errors into range data from most commercial three-dimensional range scanners, particularly scanners that are based on projected patterns and structured lighting. We study the effects of ambient light on a specific commercial scanner. We further present a method for characterizing the range accuracy as a function of ambient light distortions. After a brief review of related research, we first describe the capabilities of the scanner we used and define the experimental setup for our study. Then we present the results of the range characterization relative to ambient light. In these results, we note a systematic error source that appears to be an artifact…

Artifact (error)Opticsbusiness.industryComputer scienceOptical engineeringGeneral EngineeringRange (statistics)3d scanningStandard illuminantbusinessAtomic and Molecular Physics and OpticsStructured-light 3D scannerStructured lightOptical Engineering
researchProduct

Control systems for indoor lighting and computer simulation: analysis and comparison between software packages capabilities and results on a real cas…

2018

In the last years, computer capabilities have evolved rapidly and also the way to simulate building physics phenomena is changed and more developed. Each simulation software is developed with a less or more similar aim, using different algorithms and models and being used by people with different profile: specialist, architects, engineers, installers, etc. This paper deals with the analysis of capability of some of the most utilised software used to predict indoor lighting, including natural daylight contribution and assessment of energy consumption and savings related to specific design options. Furthermore, two of the analysed software have been tested simulating a case studying. Results …

Artificial lighting software simulation energy savings lighting design lighting control systems software reliability
researchProduct

Using machine learning to disentangle LHC signatures of Dark Matter candidates

2019

We study the prospects of characterising Dark Matter at colliders using Machine Learning (ML) techniques. We focus on the monojet and missing transverse energy (MET) channel and propose a set of benchmark models for the study: a typical WIMP Dark Matter candidate in the form of a SUSY neutralino, a pseudo-Goldstone impostor in the shape of an Axion-Like Particle, and a light Dark Matter impostor whose interactions are mediated by a heavy particle. All these benchmarks are tensioned against each other, and against the main SM background ($Z$+jets). Our analysis uses both the leading-order kinematic features as well as the information of an additional hard jet. We explore different representa…

Artificial neural network010308 nuclear & particles physicsbusiness.industryComputer sciencePhysicsQC1-999Dark matterFOS: Physical sciencesGeneral Physics and AstronomySupersymmetryMachine learningcomputer.software_genre01 natural sciencesConvolutional neural networkHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Robustness (computer science)0103 physical sciencesPrincipal component analysisProbability distributionArtificial intelligence010306 general physicsbusinessLight dark mattercomputerSciPost Physics
researchProduct

Detecting rottenness caused by Penicillium genus fungi in citrus fruits using machine learning techniques

2012

Penicillium fungi are among the main defects that may affect the commercialization of citrus fruits. Economic losses in fruit production may become enormous if an early detection of that kind of fungi is not carried out. That early detection is usually based either on UltraViolet light carried out manually. This work presents a new approach based on hyperspectral imagery for defect segmentation. Both the physical device and the data processing (geometric corrections and band selection) are presented. Achieved results using classifiers based on Artificial Neural Networks and Decision Trees show an accuracy around 98%; it shows up the suitability of the proposed approach.

Artificial neural networkbiologyComputer sciencebusiness.industryGeneral EngineeringDecision treeHyperspectral imagingMachine learningcomputer.software_genrebiology.organism_classificationComputer Science ApplicationsArtificial IntelligenceAgriculturePenicilliumUltraviolet lightArtificial intelligencebusinesscomputerExpert Systems with Applications
researchProduct

Catching the radio flare in CTA 102

2013

We performed multifrequency multiepoch Very Long Baseline Array (VLBA) observations of the blazar CTA 102 during its 2006 radio flare, the strongest ever reported for this source. These observations provide an excellent opportunity to investigate the evolution of the physical properties of blazars, especially during these flaring events. We want to study the kinematic changes in the source during the strong radio outburst in April 2006 and test the assumption of a shock-shock interaction. This assumption is based on the analysis and modeling of the single-dish observations of CTA\,102 (Paper I). In this paper we study the kinematics of CTA 102 at several frequencies using VLBI observations.…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsKinematicsAstrophysics01 natural scienceslaw.inventionlaw0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline ArrayHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomy and AstrophysicsViewing angleLight curveCTA-102Space and Planetary ScienceAstronomiaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFlareAstronomy & Astrophysics
researchProduct

Properties of the Binary Neutron Star Merger GW170817

2019

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which ar…

AstrofísicaGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsELECTROMAGNETIC COUNTERPARTspin01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESlocalization010305 fluids & plasmasGravitational wave detectorsEQUATIONenergy: densityLIGOGEO600QCastro-ph.HESettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSSettore FIS/05PhysicsEquations of stateGravitational effectsGravitational-wave signalsDeformability parameterAmplitudePhysical SciencesPhysical effectsINSPIRALING COMPACT BINARIES[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Spectral energy densityAstrophysics - High Energy Astrophysical PhenomenaPARAMETER-ESTIMATIONBinary neutron starsdata analysis methodgr-qcQC1-999Physics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesBayesianGravimeterselectromagnetic field: productionPhysics and Astronomy (all)galaxy: binary0103 physical sciencesddc:530SDG 7 - Affordable and Clean Energy010306 general physicsgravitational radiation: frequencySTFCAstrophysics::Galaxy Astrophysicsequation of stateLIGHT CURVESEquation of stateScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energySpinsgravitational radiationRCUKSpectral densityKILONOVATRANSIENTSbinary: compactStarsGEO600GalaxyLIGOgravitational radiation detectorNeutron starVIRGOPhysics and Astronomygravitational radiation: emissionRADIATIONBayesian AnalysisDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

2017

On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anticoincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of the near-simultaneous temporal and spatial observation of GRB 170817A and GW170817 occurring by chance is $5.0\times 10^{-8}$. We therefore confirm binary neutron star mergers as a progenitor of short GRBs. The association of GW170817 and GRB 170817A provides new insight into fundamental physics and the origin of short gamma-ray bursts. We use the ob…

AstrofísicaGravitacióneutron star: binaryclose [binaries]Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]BATSE OBSERVATIONSgamma-ray burst: generalEQUIVALENCE PRINCIPLEEXTENDED EMISSIONastro-ph.HE; astro-ph.HEAstrophysicsKilonovageneral [gamma-ray burst]01 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologyphoton: velocityPROMPT EMISSIONLIGOclose gamma-ray burst: general gravitational waves [binaries]gravitational wave010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)BURST SPECTRAQCQBPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)binaries: closeGRBEQUATION-OF-STATEviolation: Lorentzgamma ray: emissiongravitational wavesAstrophysics - High Energy Astrophysical PhenomenaGWradiation: electromagneticAfterglow Light CurvesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstinvariance: LorentzGW GRB LIGO Virgo Fermi BNSGLASTOptical Afterglows0103 physical sciencesgamma ray: detectorBinaries: close; gamma-ray burst: general; gravitational wavesSTFCFermi010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKAstronomy and AstrophysicsAstronomy and Astrophysictime delaysensitivityShapiro delayLIGORedshiftNeutron starVIRGOPhysics and AstronomyHOST GALAXYCPT VIOLATION13. Climate actiongravitationSpace and Planetary ScienceLUMINOSITY FUNCTIONVIEWING ANGLEbinaries: close; gamma-ray burst: general; gravitational waves; Astronomy and Astrophysics; Space and Planetary ScienceBNSspectrometerGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]redshift: measuredFermi Gamma-ray Space TelescopeAstrophysical Journal Letters
researchProduct

Determining the dark matter mass with DeepCore

2013

Cosmological and astrophysical observations provide increasing evidence of the existence of dark matter in our Universe. Dark matter particles with a mass above a few GeV can be captured by the Sun, accumulate in the core, annihilate, and produce high energy neutrinos either directly or by subsequent decays of Standard Model particles. We investigate the prospects for indirect dark matter detection in the IceCube/DeepCore neutrino telescope and its capabilities to determine the dark matter mass.

AstrofísicaNuclear and High Energy PhysicsLarge Underground Xenon experimentAstrophysics::High Energy Astrophysical PhenomenaDark matterScalar field dark matterFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesWarm dark matter010306 general physicsLight dark matterPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmologia010308 nuclear & particles physicsHot dark matterAstronomyDetectorsHigh Energy Physics - Phenomenology13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
researchProduct

The influence of circumnuclear environment on the radio emission from TDE jets

2016

Dozens of stellar tidal disruption events (TDEs) have been identified at optical, UV and X-ray wavelengths. A small fraction of these, most notably Swift J1644+57, produce radio synchrotron emission, consistent with a powerful, relativistic jet shocking the surrounding circumnuclear gas. The dearth of similar non-thermal radio emission in the majority of TDEs may imply that powerful jet formation is intrinsically rare, or that the conditions in galactic nuclei are typically unfavorable for producing a detectable signal. Here we explore the latter possibility by constraining the radial profile of the gas density encountered by a TDE jet using a one-dimensional model for the circumnuclear med…

AstrofísicaStellar populationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energylaw.inventionLuminositylaw0103 physical sciences010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)Star formationAstronomyAstronomy and AstrophysicsRadiusLight curveSynchrotronWavelength13. Climate actionSpace and Planetary ScienceAstronomiaAstrophysics - High Energy Astrophysical Phenomena
researchProduct