Search results for "Spectroscopic"

showing 10 items of 119 documents

Correcting the effect of stellar spots on ARIEL transmission spectra – II. The limb-darkening effect

2021

This paper is part of an effort to correct the transmission spectra of a transiting planet orbiting an active star. In Paper I (Cracchiolo et al. 2020) we have demonstrated a methodology to minimize the potential bias induced by unocculted star spots on the transmission spectrum, assuming a spot model parameterized by filling factor and temperature. In this work we introduce the limb darkening effect, therefore the position of the spot in the stellar disk and the impact parameter of the transiting planet now play a key role. The method is tested on simulations of planetary transits of three representative kinds of planetary systems, at ARIEL resolution. We find that a realistic treatment of…

Stars: activityFOS: Physical sciencesTechniques: spectroscopicAstrophysicsF.2.2; I.2.701 natural sciencesSpectral lineSettore FIS/05 - Astronomia E AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Earth and Planetary Astrophysics (astro-ph.EP)PhysicsPlanets and satellites: atmosphere010308 nuclear & particles physicsFilling factorI.2.7StarspotAstronomy and AstrophysicsPlanetary systemStarspotsAstrophysics - Solar and Stellar AstrophysicsTransmission (telecommunications)Space and Planetary ScienceLimb darkeningAstrophysics::Earth and Planetary AstrophysicsF.2.2Impact parameterAstrophysics - Instrumentation and Methods for AstrophysicsTechniques: photometricAstrophysics - Earth and Planetary AstrophysicsMonthly Notices of the Royal Astronomical Society
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The Gaia-ESO survey: Discovery of a spatially extended low-mass population in the Vela OB2 association

2015

The nearby (distance~350-400 pc), rich Vela OB2 association, includes $\gamma^2$ Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for investigating the formation and early evolution of young clusters. Recent Gaia-ESO survey observations have led to the discovery of two kinematically distinct populations in the young (10-15 Myr) cluster immediately surrounding $\gamma^2$ Velorum. Here we analyse the results of Gaia-ESO survey observations of NGC 2547, a 35 Myr cluster located two degrees south of $\gamma^2$ Velorum. The radial velocity distribution of lithium-rich pre-main sequence stars shows a secondary population that is kinematically distin…

Stellar populationStars: Individual: Gamma2 velorumPopulationFOS: Physical sciencesTechniques: SpectroscopicAstrophysicsVela01 natural sciencesOpen clusters and associations: Individual: NGC 25470103 physical sciencesCluster (physics)educationStars: Pre-main sequence010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QBOpen clusters and associations: Individual: Vela OB2Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsstars: formation; stars: pre-main sequence; techniques: spectroscopicAstronomy and AstrophysicRadial velocityStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStars: FormationLow MassOpen clusters and associations: Individual: NGC 2547; Open clusters and associations: Individual: Vela OB2; Stars: Formation; Stars: Individual: Gamma2 velorum; Stars: Pre-main sequence; Techniques: Spectroscopic; Astronomy and Astrophysics; Space and Planetary Science
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Clerodane diterpenoids from Salvia splendens.

2006

Four new clerodane diterpenoids, salvisplendins A-D (1-4), have been isolated from an acetone extract of the flowers of SalVia splendens, together with an artifact (5), arising from salvisplendin D (4) by addition of diazomethane, and the already known clerodane olearin (6). The structures of the new compounds (1-5) were established mainly by 1D and 2D NMR spectroscopic studies and, in the case of salvisplendin A (1), by chemical correlation with splenolide B (7). Complete 1H and 13C NMR assignments for olearin (6), not published hitherto, are also reported.

StereochemistryPharmaceutical ScienceFlowersSalviaAnalytical ChemistryDiterpenes Clerodanechemistry.chemical_compoundFour new clerodane diterpenoids salvisplendins A-D (1-4) have been isolated from an acetone extract of the flowers of SalVia splendens together with an artifact (5) arising from salvisplendin D (4) by addition of diazomethane and the already known clerodane olearin (6). The structures of the new compounds (1-5) were established mainly by 1D and 2D NMR spectroscopic studies and in the case of salvisplendin A (1) by chemical correlation with splenolide B (7). Complete 1H and 13C NMR assignments for olearin (6) not published hitherto are also reportedDrug DiscoveryOrganic chemistrySalviaNuclear Magnetic Resonance BiomolecularPharmacologychemistry.chemical_classificationPlants MedicinalbiologyMolecular StructureChemistryDiazomethaneOrganic ChemistryCarbon-13 NMRbiology.organism_classificationChemical correlationTerpenoidComplementary and alternative medicineItalyMolecular MedicineDiterpeneTwo-dimensional nuclear magnetic resonance spectroscopyLactoneJournal of natural products
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La pittura vascolare attica a fondo bianco: la prospettiva archeologica, l'apporto dell'indagine scientifica

2017

Il presente contributo intende offrire nuovi spunti di ricerca sui vasi attici a fondo bianco e sulla relativa tecnica pittorica. In particolare, è stato selezionato come caso di studio il cratere del Pittore della Phiale (450-440 a.C.) con il mito di Perseo e Andromeda, esposto nel Museo Archeologico di Agrigento. La prima parte del lavoro si concentra sugli aspetti archeologici e storico-artistici, cercando di ricostruire il ruolo di questa tecnica nella produzione figurativa dell’artigiano e il rapporto tra il cratere di Agrigento e gli altri prodotti del Pittore della Phiale. Inoltre, viene considerata la connessione tra tecnica e con- testo di utilizzo e acquirenti o “committenti”, la…

Tecnica a fondo bianco Agrigento Pittore della Phiale analisi spettroscopiche fluoriescenza a raggi X TR-FTIR.Settore L-ANT/07 - Archeologia ClassicaWhite-ground technique Agrigento Phiale Painter spectroscopic analysis X-ray fluorescence TR-FTIRSettore CHIM/02 - Chimica Fisica
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Charge Sharing and Cross Talk Effects in High-Z and Wide-Bandgap Compound Semiconductor Pixel Detectors

2023

Intense research activities have been made in the development of high-Z and wide-bandgap compound semiconductor pixel detectors for the next generation X-ray and gamma ray spectroscopic imagers. Cadmium telluride (CdTe) and cadmium-zinc-telluride (CdZnTe or CZT) pixel detectors have shown impressive performance in X-ray and gamma ray detection from energies of few keV up to 1 MeV. Charge sharing and cross-talk phenomena represent the typical drawbacks in sub-millimeter pixel detectors, with severe distortions in both energy and spatial resolution. In this chapter, we review the effects of these phenomena on the response of CZT/CdTe pixel detectors, with particular emphasis on the current st…

X-ray and gamma ray detectorsCdZnTe detectorsCompound semiconductor detectorsCross talkSpectroscopic X-ray imagingSettore FIS/01 - Fisica SperimentaleCharge sharingSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)CdTe detectors
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X‐Ray Photoelectron Spectroscopy

2021

X-ray photoelectron spectroscopy (XPS) is a spectroscopic technique in the family of electron spectroscopies, that is, those methods whose probe consists of electrons instead of photons. In the case of XPS, a soft, usually monochromatic X-ray causes the emission of electrons by means of the photoelectric effect. Differences in chemical potential and/or polarizability of the molecules can cause an alteration of the binding energy; in addition to photoelectrons, an ordinary XPS spectrum may also contain Auger electrons. In an XPS system, an electron gun is used to deliver a low-energy electron flux with a low current over the illuminated spot. In an XPS instrument, an ion gun may be used with…

X-ray photoelectron spectroscopyMaterials scienceX-ray photoelectron spectroscopyPhotoelectric effectSettore CHIM/03 - Chimica Generale E InorganicaAnalytical chemistryElectron spectroscopySpectroscopic techniqueAuger electronsBinding energySpectroscopy for Materials Characterization
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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On the high resolution spectroscopy and intramolecular potential function of SO2

2009

Abstract Two weak stretching bands, ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , of the sulfur dioxide molecule have been recorded at high resolution and analyzed for the first time with using a Fourier transform Bruker IFS-120 HR interferometer. About 1000 transitions with J max .  = 51, K a max . = 16 , and 900 transitions with J max .  = 53, K a max . = 16 have been assigned to the bands ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , respectively. Analysis of the recorded spectra was made using the model of isolated vibrational states. Parameters obtained from the fit reproduce the initial experimental ro-vibrational energies with the rms deviation of 0.0006 and 0.0012 cm −1 for the bands, 3 ν 1  +  ν 3 and ν 1  …

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Analytical chemistryHigh resolution02 engineering and technology01 natural sciencesSpectral linesymbols.namesakeNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]High-resolution spectra0103 physical sciencesMoleculePhysical and Theoretical ChemistrySpectroscopySpectroscopyPhysics010304 chemical physicsPotential functionFunction (mathematics)Spectroscopic parameters021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsInterferometryFourier transformSulfur dioxideIntramolecular forcesymbols0210 nano-technology
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High resolution study of the six lowest doubly excited vibrational states of PH2D

2005

Abstract The five lowest doubly excited deformational vibrational bands ν 4  +  ν 6 , 2 ν 6 , ν 3  +  ν 4 , ν 3  +  ν 6 , and 2 ν 3 of PH 2 D have been recorded for the first time using a Bruker 120 HR interferometer with a resolution 0.0033 cm −1 and analysed. Some transitions belonging to a very weak band 2 ν 4 have been also assigned. From the fit 24 and 86, respectively, diagonal and resonance interaction parameters were obtained which reproduce 1089 upper energy levels obtained from more than 4600 assigned transitions with the rms deviation of 0.00059 cm −1 .

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]InfraredHigh resolution010402 general chemistry01 natural sciencesNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesVibrational bandsHigh resolutionPhysical and Theoretical ChemistryInfrared spectrumSpectroscopy[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Physics010304 chemical physicsResolution (electron density)ResonanceSpectroscopic parametersPH2D moleculeAtomic and Molecular Physics and Optics0104 chemical sciences[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]FTIRExcited stateAtomic physics
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Analysis of highly excited 'hot' bands in the SO2 molecule: ν2 + 3ν3 - ν2 and 2ν1 + ν2 + ν3 - ν2

2010

International audience; We set up a variational procedure of assignments of transitions and we applied it to the analysis very weak 'hot' bands, v(2) + 3v(3) - v(2) and 2v(1) + v(2) + v(3) - v(2), of the SO2 molecule. As the first step of the study, the 'cold' bands, 3v(3) and 2v(1) + v(3), are re-analysed and transitions belonging to those bands are assigned up to the values of quantum numbers J(max.) = 60, K-a(max.) = 19, and J(max.) = 69, K-a(max.) = 20 for the bands 3v(3) and 2v(1) + v(3), respectively. After 'cleaning' the experimental spectrum from transitions belonging to the 3v(3) and 2v(1) + v(3) bands, a variational procedure was used that allowed us to assign 230 and 115 transiti…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]high-resolution spectraHIGH-RESOLUTION ANALYSISBiophysics02 engineering and technology01 natural sciences[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesMoleculespectroscopic parametersHigh resolution spectraPhysical and Theoretical ChemistrySpectroscopyLASER SPECTROSCOPYMolecular BiologyHigh resolution analysis010304 chemical physicsChemistryCOMBINATION BAND021001 nanoscience & nanotechnologyCondensed Matter PhysicsQuantum numberNU-3 BANDINTENSITIESSULFUR-DIOXIDEExcited stateLINE POSITIONSVIBRATIONAL-STATESsulphur dioxideEQUILIBRIUM ROTATIONAL-CONSTANTSAtomic physics0210 nano-technologySUBMILLIMETER-WAVE SPECTRUM
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