Search results for "SPECTROSCOPIC"

showing 10 items of 119 documents

The STDS Dijon system : Present status and prospects.

2009

The Dijon spectroscopy group has developed powerful techniques based on group theory and tensorial formalism in order to analyze and simulate absorption and Raman spectra of molecules with various symmetries. Software packages and databases implementing these tools have been created [1]. Compared to the widely used spectroscopic databases (HITRAN, GEISA), these packages, with their XTDS common interface [2], are primarily devoted to the calculation of line parameters and spectra from a database of model parameters. Future developments include improved fitting algorithms, inclusion of C3v symmetric tops, rovibronic couplings, uncertainty estimates. Moreover, calculated line lists will be acc…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Computational spectroscopymethanespectroscopic database[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
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ESPRESSO highlights the binary nature of the ultra-metal-poor giant HE 0107-5240

2020

Context. The vast majority of the known stars of ultra low metallicity ([Fe=H] >-4:5) are known to be enhanced in carbon, and belong to the 'low-carbon band' (A(C) = log(C=H) + 12 7:6). It is generally, although not universally, accepted that this peculiar chemical composition reflects the chemical composition of the gas cloud out of which these stars were formed. The first ultra-metalpoor star discovered, HE 0107-5240, is also enhanced in carbon and belongs to the 'low-carbon band'. It has recently been claimed to be a long-period binary, based on radial velocity measurements. It has also been claimed that this binarity may explain its peculiar composition as being due to mass transfer fro…

[PHYS]Physics [physics]Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsBinary numberabundances [Galaxy]Astronomy and AstrophysicsAstrophysics01 natural sciencesGalactic haloEspressospectroscopic [Binaries]Space and Planetary Scienceabundances [Stars]0103 physical scienceshalo [Galaxy]Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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Chemometric Tools to Point Out Benchmarks and Chromophores in Pigments through Spectroscopic Data Analyses

2021

Spectral preprocessing data and chemometric tools are analytical methods widely applied in several scientific contexts i.e., in archaeometric applications. A systematic classification of natural powdered pigments of organic and inorganic nature through Principal Component Analysis with a multi-instruments spectroscopic study is presented here. The methodology allows the access to elementary and molecular unique benchmarks to guide and speed up the identification of an unknown pigment and its recipe. This study is conducted on a set of 48 powdered pigments and tested on a real-case sample from the wall painting in S. Maria Delle Palate di Tusa (Messina, Italy). Four spectroscopic techniques …

ancient pigmentsspectroscopic techniquesOrganic ChemistryPharmaceutical Scienceancient pigments; spectroscopic techniques; chemometrics discrimination; elemental and molecular benchmarksArticlechemometrics discriminationAnalytical Chemistryelemental and molecular benchmarksQD241-441Chemistry (miscellaneous)Drug DiscoveryMolecular MedicinePhysical and Theoretical ChemistryMolecules; Volume 27; Issue 1; Pages: 163
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HADES RV programme with HARPS-N at TNG: XII. The abundance signature of M dwarf stars with planets

2020

[Context] Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing.

astro-ph.SRStellar massMetallicityFOS: Physical sciencesTechniques: spectroscopicStars: late-typeAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesspectroscopic [Techniques]Settore FIS/05 - Astronomia E AstrofisicaPrimary (astronomy)PlanetAbundance (ecology)0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsEarth and Planetary Astrophysics (astro-ph.EP)Physics010308 nuclear & particles physicsStars: abundancesGiant planetAstronomy and Astrophysicsastro-ph.SR; astro-ph.SR; astro-ph.EPRadial velocityStarsPlanetary systemsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Scienceabundances [Stars]late-type [Stars]astro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
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Neutron halos in the excited states of 12B

2018

The differential cross sections of the 11B(d,p) 12B reaction leading to formation of the 1+ ground state and the 0.95-MeV 2+, 1.67-MeV 2−, 2.62-MeV 1−, 2.72-MeV 0+, and 3.39-MeV 3− excited states of 12B are measured at Ed = 21.5 MeV. The analysis of the data is carried out within the coupled-reaction-channels method for the direct neutron transfer and the Hauser-Feshbach formalism of the statistical compound-nucleus model. The spectroscopic factors, asymptotic normalization coefficients, and rms radii of the last neutron in all states studied are deduced. The existence of the neutron halos in the 1.67-MeV 2− and 2.62-MeV 1− states is found, consistent with the earlier published data. New in…

cluster modelselectromagnetic momentsNuclear Theorynucleon distributiontransfer reactionsbooriPhysics::Accelerator Physicsspectroscopic factorsdirect reactionsNuclear Experimentydinfysiikka
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Clusterization and Strong Coulpled-Channels Effects in Deuteron Interaction with 9Be Nuclei

2019

Angular distributions of protons, deuterons, tritons and alphaparticles emitted in the d + 9Be reaction at Elab=19.5 and 35.0 MeV have been measured. The elastic scattering channel is analysed in the framework of both the Optical Model and the Coupled-Channel approach. The interaction potential of the d + 9Be system is calculated in the framework of the Double-Folding model using the α + α + n three-body wave function of the 9Be nucleus. The (d, p) and (d, t) one-nucleon-transfer reactions are analysed within the coupledreaction-channel approach. The spectroscopic amplitudes for the different nuclear cluster configurations are calculated. Differential cross sections for the reaction channel…

double foldingelastic and inelastic scatteringNuclear Theoryoptical modelDWBAfew-nucleon transfer reactionshiukkasfysiikkaNuclear Experimentydinfysiikkaspectroscopic amplitudescluster structureCRC
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On the local mode behaviour of the XH2/XD2 and XD/XH fragments with respect to the deuterated species of the near local mode XH3(C3v ) molecule

2009

International audience; Effect of isotopic substitution in the near local mode, XH3(C3v), molecules is considered. On that basis it is shown that the spectroscopic properties of deuterated and/or di-deuterated isotopic species of the XH3(C3v) molecule with the value of interbond angle close to π/2 are analogous to the spectroscopic properties of its separate fragments: of a three-atomic local mode 'molecule' XH2/XD2 and of a diatomic XD/XH 'molecule'. The phosphine molecule is considered as an illustration.

isotopic substitution010304 chemical physics[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]ChemistryBiophysicsMode (statistics)local mode model010402 general chemistryCondensed Matter Physics01 natural sciencesDiatomic molecule0104 chemical sciencesCrystallographychemistry.chemical_compoundDeuterium[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Computational chemistry0103 physical sciencesMoleculespectroscopic parametersPhysical and Theoretical ChemistryMolecular BiologyPhosphine
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Fusingin vivoandex vivoNMR sources of information for brain tumor classification

2011

In this study we classify short echo-time brain magnetic resonance spectroscopic imaging (MRSI) data by applying a model-based canonical correlation analyses algorithm and by using, as prior knowledge, multimodal sources of information coming from high-resolution magic angle spinning (HR-MAS), MRSI and magnetic resonance imaging. The potential and limitations of fusing in vivo and ex vivo nuclear magnetic resonance sources to detect brain tumors is investigated. We present various modalities for multimodal data fusion, study the effect and the impact of using multimodal information for classifying MRSI brain glial tumors data and analyze which parameters influence the classification results…

medicine.diagnostic_testComputer sciencebusiness.industryApplied MathematicsMultimodal dataBrain tumorMagnetic resonance spectroscopic imagingMagnetic resonance imagingPattern recognitionmedicine.diseaseNuclear magnetic resonanceIn vivomedicineMagic angle spinningBrain magnetic resonance imagingArtificial intelligencebusinessInstrumentationEngineering (miscellaneous)Ex vivoMeasurement Science and Technology
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Differentiation between brain metastases and glioblastoma multiforme based on MRI, MRS and MRSI

2009

Brain metastases and glioblastoma multiforme are the most aggressive and common brain tumours in adults and they require a different clinical management. Anatomical magnetic resonance imaging (MRI) or clinical history, cannot always clearly distinguish between them. This study describes and verifies the use of magnetic resonance spectroscopy (MRS) and magnetic resonance spectroscopic imaging (MRSI) in combination with MRI for differential diagnosis of glioblastomas and metastases. Feature selection methods are applied to the magnetic resonance (MR) spectra of 121 patients and relevant features are detected. Different classification methods are used to distinguish glioblastoma multiforme and…

medicine.medical_specialtymedicine.diagnostic_testbusiness.industryMagnetic resonance spectroscopic imagingMagnetic resonance imagingmedicine.diseaseMetastasisClinical historymedicineRadiologyDifferential diagnosisMr imagesbusinessBrain metastasisGlioblastoma
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