Search results for "Spectral line"

showing 10 items of 1453 documents

<title>Micro-Raman scattering and infrared spectra of hemoglobin</title>

2008

Confocal micro-Raman and FT-IR spectroscopies have been used for detection of radiation influence of hemoglobin of patients examined by radio-isotopes diagnosis (Tc99m). After irradiation we observed some little changes of the Raman scattering bands which connected with out of plane porphyrine bending vibrations, also we observed additional band due to methemoglobin. Radiation of blood lead to the transition from hemoglobin (Fe2+) to methemoglobin (Fe3+) with a delocalization of iron from porphyrine plane. It was shown that FT-IR spectra indicate the radiation effects on hemoglobin.© (2008) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is per…

inorganic chemicalsScatteringChemistryAnalytical chemistryInfrared spectroscopyMethemoglobinSpectral lineFourier transform spectroscopysymbols.namesakeNuclear magnetic resonancesymbolsIrradiationHemoglobinRaman scatteringSPIE Proceedings
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Global analysis of the high resolution infrared spectrum of methane 12CH4 in the region from 0 to 4800 cm-1

2009

International audience; We report the global analysis of methane (12CH4) lines from high resolution rovibrational spectra including accurate line positions and intensities in the region 0–4800 cm−1. This covers four polyads: The Ground State Monad (rotational levels), the Dyad (940–1850 cm−1, 2 vibrational levels, 2 sublevels), the Pentad (2150–3350 cm−1, 5 vibrational levels, 9 sublevels) and the Octad (3550–4800 cm−1, 8 vibrational levels, 24 sublevels) and some of the associated hot bands (Pentad−Dyad and Octad−Dyad). New Fourier transform infrared (FTIR) spectra of the Pentad and Octad regions have been recorded with a very high resolution (better than 0.001 cm−1 instrumental bandwidth,…

line intensitiesInfraredGeneral Physics and Astronomy02 engineering and technology01 natural sciencesSpectral lineRoot mean squaresymbols.namesakehigh resolution infrared spectra0103 physical sciencesPhysical and Theoretical Chemistry[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]010304 chemical physicsSpectrometerChemistryRotational–vibrational spectroscopy021001 nanoscience & nanotechnologyPotential energyFourier transform[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]symbolsrovibrational analysisAtomic physics0210 nano-technologyGround stateMethanevibrational states
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Long-term monitoring of the TeV emission from Mrk 421 with the ARGO-YBJ experiment

2011

ARGO-YBJ is an air shower detector array with a fully covered layer of resistive plate chambers. It is operated with a high duty cycle and a large field of view. It continuously monitors the northern sky at energies above 0.3 TeV. In this paper, we report a long-term monitoring of Mrk 421 over the period from 2007 November to 2010 February. This source was observed by the satellite-borne experiments Rossi X-ray Timing Explorer and Swift in the X-ray band. Mrk 421 was especially active in the first half of 2008. Many flares are observed in both X-ray and gamma-ray bands simultaneously. The gamma-ray flux observed by ARGO-YBJ has a clear correlation with the X-ray flux. No lag between the X-r…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaOggetti di tipo BL LacertaeFOS: Physical sciencesFluxAstrophysics01 natural sciences7. Clean energyindividual (Markarian 421) [BL Lacertae objects]Spectral lineGamma-rays Markarian 421 BL Lacertae Resistive Plate Chamberslaw.inventionlaw0103 physical sciencesRadiative transfer010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsMarkarian 421Settore FIS/01 - Fisica SperimentaleAstronomy and Astrophysicsgeneral [gamma ray]Synchrotron3. Good healthAir shower13. Climate actionSpace and Planetary ScienceDuty cycleSkyRaggi gammaSpectral energy distributionAstrophysics - High Energy Astrophysical Phenomena
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Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006

2018

We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN. We extract the NuSTAR spectra from a few regions along the non-thermal limbs and jointly analyze them with the XMM-Newton spectra and the radio data. The broad-band radio/X-ray spectra can be well described with a synchrotron emission model from a single population of CR electrons with a power law energy distribution and an exponential cutoff. The power law index of the electron particle distribution function (PDF) is ~1.88-1.95 for both the NE and SW l…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryPower lawSpectral linecosmic rays0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumeducation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonISM: supernova remnantsacceleration of particlesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsshock wavesAstronomy and Astrophysicradiation mechanisms: non-thermalX-rays: ISMMagnetic fieldSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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Snapshot multi-spectral-line imaging for applications in dermatology and forensics

2019

Performance of multi-spectral imaging critically depends on image acquisition time and working spectral bandwidths. Ultimate performance can be achieved if a set of monochromatic (single-wavelength) spectral images is obtained by a single snapshot - a technique provisionally called “snapshot multi-spectral-line imaging” or SMSLI. The SMSLI principle and the developed prototype devices for 3, 4 and 5 spectral line snapshot imaging are described. Two potential practical applications of SMSLI are discussed – for fast mapping of the main in-vivo skin chromophores and for detection of counterfeit banknotes and documents.

medicine.medical_specialtyComputer sciencebusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONMulti spectralSpectral lineSpectral imagingmedicineImage acquisitionSnapshot (computer storage)Computer visionMonochromatic colorArtificial intelligencebusinessImaging, Manipulation, and Analysis of Biomolecules, Cells, and Tissues XVII
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Laser illumination designs for snapshot multi-spectral-line imaging

2019

For multi-spectral imaging, both acquisition time of the spectral image set and the spectral bandwidth of each image have to be minimized. Ultimate performance can be achieved if the set of monochromatic (single-wavelength) spectral images is obtained with a single snapshot — a technique provisionally called "snapshot multi-spectral-line imaging" or SMSLI. Using contemporary RGB colour cameras, up to three spectral line images can be extracted from a snapshot image data cube at specific illumination that comprises only three spectral lines, each of them positioned within one of the detection bands (R, G or B) [1]. Techniques able to provide more spectral line images are under development, a…

medicine.medical_specialtyComputer sciencebusiness.industryData_MISCELLANEOUSMultispectral imageComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONLaser01 natural sciencesSpectral linelaw.inventionSpectral imaging010309 opticsData cubeOpticslawComputer Science::Computer Vision and Pattern Recognition0103 physical sciencesmedicineRGB color modelSnapshot (computer storage)Monochromatic colorbusiness
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Single snapshot RGB multispectral imaging at fixed wavelengths: proof of concept

2014

A concept of single snapshot multispectral imaging by standard RGB image sensors under spectrally-specific illumination comprising a fixed number of narrow spectral lines is discussed and experimentally validated. The limiting conditions, RGB band spectral crosstalk corrections and potential applications for parametric mapping of skin are regarded, along with the preliminary results of the proof-of-concept measurements.

medicine.medical_specialtyComputer sciencebusiness.industryMultispectral imageSpectral lineSpectral imagingWavelengthOpticsProof of conceptComputer Science::Computer Vision and Pattern RecognitionmedicineRGB color modelSnapshot (computer storage)businessParametric statisticsSPIE Proceedings
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Model, software and database for line-mixing effects in the ν3 and ν4 bands of CH4 and tests using laboratory and planetary measurements-I: N2(and ai…

2006

International audience; Absorption spectra of the infrared ν3 and ν4 bands of CH4 perturbed by N2 over large ranges of pressure and temperature have been measured in the laboratory. A theoretical approach accounting for line mixing is proposed to (successfully) model these experiments. It is similar to that of Pieroni et al. [J Chem Phys 1999;110:7717–32] and is based on state-to-state rotational cross-sections calculated with a semi-classical approach and a few empirical parameters. The latter, which enable switching from the state space to the line space, are deduced from a fit of a single room temperature spectrum of the ν3 band at 50 atm. The comparisons between numerous measured and ca…

methane infrared spectra atmotspheric absorptionRadiationMaterials science010504 meteorology & atmospheric sciencesDatabaseAbsorption spectroscopy[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]computer.software_genre01 natural sciencesAtomic and Molecular Physics and OpticsSpectral line010309 opticssymbols.namesakeAtmosphere of EarthFourier transform13. Climate action0103 physical sciencesRadiative transfersymbolsEmission spectrumAbsorption (electromagnetic radiation)computerSpectroscopy0105 earth and related environmental sciencesLine (formation)
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A magnetic look into the protecting layer of Au25 clusters

2016

The field of molecular metal clusters protected by organothiolates is experiencing a very rapid growth. So far, however, a clear understanding of the fine interactions between the cluster core and the capping monolayer has remained elusive, despite the importance of the latter in interfacing the former to the surrounding medium. Here, we describe a very sensitive methodology that enables comprehensive assessment of these interactions. Pulse electron nuclear double resonance (ENDOR) was employed to study the interaction of the unpaired electron with the protons of the alkanethiolate ligands in four structurally related paramagnetic Au25(SR)0 18 clusters (R ¼ ethyl, propyl, butyl, 2-methylpro…

molecular metal clusterselectronic distributionkemiaIcosahedral symmetryAnalytical chemistry02 engineering and technologychemistry010402 general chemistrygold clusters01 natural sciencesSpectral lineAu25ParamagnetismMolecular dynamicsNMR spectroscopyMonolayerthiolate-cappedCluster (physics)ta116Electron nuclear double resonanceChemistryChemistry (all)paramagnetic gols nanoclustersGeneral ChemistryENDOR spectroscopy021001 nanoscience & nanotechnology0104 chemical sciencesUnpaired electronChemical physics0210 nano-technology
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Bright Visible Luminescence in Silica Nanoparticles

2011

International audience; We demonstrate that a porous film of silica nanoparticles emits a bright visible luminescence associated with defects stabilized by oxygen chemisorption at oxygen deficient center sites. Time-resolved spectra excited by a tunable laser allow us to distinguish the luminescence at 1.99 eV, characteristic of the nonbridging oxygen hole center (NBOHC) (Si-O)3 Si-O*, and a fast and a slow emission: the first (lifetime τ ≈ 25 ns) is peaked at 2.27 eV with an excitation spectrum centered at 5.5 eV; the second (τ ≈ 7.5 μs) is peaked at 2.41 eV and is excited around 3.2 and 5.2 eV. Reaction in an air atmosphere leads to the disappearance of the NBOHC luminescence and of the …

nanoparticles silica time resolved luminescence[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Materials scienceSilanoneNanoparticleSpectral lineSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsGeneral EnergyChemisorptionExcited statePhysical and Theoretical ChemistryAtomic physicsLuminescenceExcitationTunable laserThe Journal of Physical Chemistry C
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