Search results for "Spectrum"

showing 10 items of 2043 documents

Structural and Dynamic Properties of the Homodimeric Hemoglobin from Scapharca inaequivalvis Thr-72→Ile Mutant: Molecular Dynamics Simulation, Low Te…

1998

AbstractMolecular dynamics simulations, low temperature visible absorption spectroscopy, and resonance Raman spectroscopy have been performed on a mutant of the Scapharca inaequivalvis homodimeric hemoglobin, where residue threonine 72, at the subunit interface, has been substituted by isoleucine. Molecular dynamics simulation indicates that in the Thr-72→Ile mutant several residues that have been shown to play a role in ligand binding fluctuate around orientations and distances similar to those observed in the x-ray structure of the CO derivative of the native hemoglobin, although the overall structure remains in the T state. Visible absorption spectroscopy data indicate that in the deoxy …

Absorption spectroscopyProtein subunitDimerResonance Raman spectroscopyMutantBiophysicsHemeSpectrum Analysis Ramanchemistry.chemical_compoundHemoglobinsMutant proteinAnimalsHemeHistidineCarbon MonoxideChemistrySettore BIO/11TemperatureWaterCrystallographyMolluscaSpectrophotometryMutationDimerizationProtein BindingResearch ArticleBiophysical Journal
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On the Low-Lying Excited States ofsym-Triazine-Based Herbicides

2005

We report a joint computational and luminescence study on the low-lying excited states of sym-triazines, namely, 1,3,5-triazine (1) and the ubiquitous herbicides atrazine [6-chloro-N2-ethyl-N4-isopropyl-1,3,5-triazine-2,4-diamine (2)] and ametryn [6-methylthio-N2-ethyl-N4-isopropyl-1,3,5-triazine-2,4-diamine (3)]. Geometrical structures, energetics, and transition and state properties of I and 2 were computed at the TD-DFT, CASSCF, and CASPT2 levels of theory. The fluorescence and phosphorescence emission spectra, lifetimes, and fluorescence quantum yields were measured for the three compounds, and from these, the energies of the lowest excited states and their corresponding radiative rates…

Absorption spectroscopyQuantum yieldPhotochemistryMolecular physicsAbsorptionAb initio quantum chemistry methodsOscillometryPressureRadiative transferEmission spectrumPhysical and Theoretical ChemistryMolecular StructureChemistry PhysicalHerbicidesTriazinesChemistryTemperatureHydrogen-Ion ConcentrationModels TheoreticalAtomic and Molecular Physics and OpticsSpectrometry FluorescenceModels ChemicalSpectrophotometryExcited stateAtrazineIndicators and ReagentsPhosphorescenceLuminescenceSoftwareChemPhysChem
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Absorption spectrum of the and electronic transitions of ReF6

1999

Abstract The absorption spectra of the near-infrared and ultraviolet bands of ReF6 have been recorded with a commercial spectrophotometer. The vibronic assignments previously published by different authors are critically revised. A non-perturbative method has been used to calculate the linear Jahn–Teller levels for the ν5 mode in the ground electronic state. Some new vibronic parameter values are derived. The ν5 linear Jahn–Teller parameter in the X G′ g electronic state is found to be D5=0.103(9). The ultraviolet absorption spectrum has enabled us to determine relatively accurate values of the crystal-field (10Dq) and spin-orbit (ζd) parameters.

Absorption spectroscopyRhenium hexafluoridemedicine.disease_causeAtomic and Molecular Physics and OpticsUltraviolet absorption spectrumAnalytical Chemistrychemistry.chemical_compoundchemistryAtomic electron transitionmedicineVibronic spectroscopyCondensed Matter::Strongly Correlated ElectronsAtomic physicsInstrumentationSpectroscopyUltravioletSpectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy
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Transition-Edge Sensors for Particle Induced X-ray Emission Measurements

2013

In this paper we present a new measurement setup, where a transitionedge sensor detector array is used to detect X-rays in particle induced X-ray emission measurements with a 2 MeV proton beam. Transition-edge sensors offer orders of magnitude improvement in energy resolution compared to conventional silicon or germanium detectors, making it possible to recognize spectral lines in materials analysis that have previously been impossible to resolve, and to get chemical information from the elements. Our sensors are cooled to the operation temperature (65 mK) with a cryogen-free adiabatic demagnetization refrigerator, which houses a specially designed X-ray snout that has a vacuum tight window…

Accelerator Physics (physics.acc-ph)Physics - Instrumentation and DetectorsMaterials scienceProtonPhysics::Instrumentation and DetectorsOrders of magnitude (temperature)FOS: Physical scienceschemistry.chemical_elementGermaniumRadiationSpectral lineOpticsGeneral Materials Scienceparticle induced X-ray emission (PIXE)Emission spectrumbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)transition-edge sensorCondensed Matter PhysicsAtomic and Molecular Physics and OpticsFull width at half maximumchemistryPhysics - Accelerator PhysicsbusinessTESJournal of Low Temperature Physics
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Spectral and timing properties of IGR J00291+5934 during its 2015 outburst

2016

We report on the spectral and timing properties of the accreting millisecond X-ray pulsar IGR J00291+5934 observed by XMM-Newton and NuSTAR during its 2015 outburst. The source is in a hard state dominated at high energies by a comptonization of soft photons ($\sim0.9$ keV) by an electron population with kT$_e\sim30$ keV, and at lower energies by a blackbody component with kT$\sim0.5$ keV. A moderately broad, neutral Fe emission line and four narrow absorption lines are also found. By investigating the pulse phase evolution, we derived the best-fitting orbital solution for the 2015 outburst. Comparing the updated ephemeris with those of the previous outbursts, we set a $3��$ confidence leve…

AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesPulsar0103 physical sciencesneutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion; Accretion discs; Stars]Emission spectrumSpectroscopy010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodX-rays: binarieStars: neutronNeutron starAmplitude13. Climate actionSpace and Planetary ScienceAccretion discAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)Monthly Notices of the Royal Astronomical Society
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Redshifted X-rays from the material accreting onto TW Hya: evidence of a low-latitude accretion spot

2017

High resolution spectroscopy, providing constraints on plasma motions and temperatures, is a powerful means to investigate the structure of accretion streams in CTTS. In particular, the accretion shock region, where the accreting material is heated to temperatures of a few MK as it continues its inward bulk motion, can be probed by X-ray spectroscopy. To attempt to detect for the first time the motion of this X-ray-emitting post-shock material, we searched for a Doppler shift in the deep Chandra/HETGS observation of the CTTS TW Hya. This test should unveil the nature of this X-ray emitting plasma component in CTTS, and constrain the accretion stream geometry. We searched for a Doppler shift…

AccretionTechniques: spectroscopicFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesTW HydraeX-rays: starEmission spectrumSpectroscopy010303 astronomy & astrophysicsStars: variables: T TauriSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPhotosphereLine-of-sight010308 nuclear & particles physicsHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicRedshiftAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsAccretion diskSpace and Planetary ScienceStars: pre-main sequence
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Measurement of acoustic attenuation in South Pole ice

2010

Using the South Pole Acoustic Test Setup (SPATS) and a retrievable transmitter deployed in holes drilled for the IceCube experiment, we have measured the attenuation of acoustic signals by South Pole ice at depths between 190 m and 500 m. Three data sets, using different acoustic sources, have been analyzed and give consistent results. The method with the smallest systematic uncertainties yields an amplitude attenuation coefficient alpha = 3.20 \pm 0.57 km^(-1) between 10 and 30 kHz, considerably larger than previous theoretical estimates. Expressed as an attenuation length, the analyses give a consistent result for lambda = 1/alpha of ~1/300 m with 20% uncertainty. No significant depth or …

Acoustic attenuation; Acoustics; Ice; Neutrino astronomy; South Pole[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]010504 meteorology & atmospheric sciences[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]iceFOS: Physical sciencesAetiology screening and detection [ONCOL 5]Lambda01 natural sciencesneutrino astronomy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrum0103 physical sciencesacousticsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesPhysicsSouth Pole010308 nuclear & particles physicsbusiness.industryAttenuation[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TransmitterAttenuation lengthAstronomy and AstrophysicsGeodesy004AmplitudeAttenuation coefficientddc:540NeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsbusinessAcoustic attenuationinfo:eu-repo/classification/ddc/004acoustic attenuation
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Model Predictive Control for Shunt Active Filters With Fixed Switching Frequency

2016

This paper presents a modification to the classical Model Predictive Control algorithm, named Modulated Model Predictive Control, and its application to active power filters. The proposed control is able to retain all the advantages of a Finite Control Set Model Predictive Control whilst improving the generated waveforms harmonic spectrum. In fact a modulation algorithm, based on the cost function ratio for different output vectors, is inherently included in the MPC. The cost function-based modulator is introduced and its effectiveness on reducing the current ripple is demonstrated. The presented solution provides an effective and straightforward single loop controller, maintaining an excel…

Active filters; harmonic distortion; model predictive control (MPC); power filters; power quality; smart gridsEngineeringmodel predictive control (MPC)020209 energyRipple02 engineering and technologyIndustrial and Manufacturing EngineeringHarmonic analysisHarmonic spectrumControl theory0202 electrical engineering electronic engineering information engineeringElectronic engineeringsmart gridsWaveformElectrical and Electronic EngineeringActive filterModel Predictive ControlActive filtersTotal harmonic distortionbusiness.industry020208 electrical & electronic engineeringpower filtersAC powerpower qualityharmonic distortionModel predictive controlControl and Systems Engineeringbusiness
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Extended X-ray emission in PKS 1718-649

2018

PKS 1718$-$649 is one of the closest and most comprehensively studied candidates of a young active galactic nucleus (AGN) that is still embedded in its optical host galaxy. The compact radio structure, with a maximal extent of a few parsecs, makes it a member of the group of compact symmetric objects (CSO). Its environment imposes a turnover of the radio synchrotron spectrum towards lower frequencies, also classifying PKS 1718$-$649 as gigahertz-peaked radio spectrum (GPS) source. Its close proximity has allowed the first detection of extended X-ray emission in a GPS/CSO source with Chandra that is for the most part unrelated to nuclear feedback. However, not much is known about the nature …

Active galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumlaw.inventionlawIonization0103 physical sciences010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsStar formationAntenna apertureAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesSynchrotronGalaxySupernovaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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Wind-luminosity evolution in NLS1 AGN 1H 0707−495

2021

Ultra-fast outflows (UFOs) have been detected in the high-quality X-ray spectra of a number of active galactic nuclei (AGN) with fairly high accretion rates and are thought to significantly contribute to the AGN feedback. After a decade of dedicated study, their launching mechanisms and structure are still not well understood, but variability techniques may provide useful constraints. In this work, therefore, we perform a flux-resolved X-ray spectroscopy on a highly accreting and variable NLS1 AGN, 1H 0707-495, using all archival XMM-Newton observations to study the structure of the UFO. We find that the wind spectral lines weaken at higher luminosities, most likely due to an increasing ion…

Active galactic nucleusAstrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineLuminosityaccretionIonization0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsRadiusaccretion discsgalaxies: SeyfertSpace and Planetary ScienceX-rays: individual: 1H 0707−495OutflowAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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