Search results for "WAVELENGTH"

showing 10 items of 741 documents

Synthesis and Electronic Spectra of Substitutedp-Distyrylbenzenes for the Use in Light-Emitting Diodes

2000

The influence of substitution on the absorption and Luminescence spectra of oligo(phenylenevinylene)s has been studied using distyrylbenzene (DSB) as a model compound. The degree, character, and pattern of substitution was varied systematically, altering the electronic properties of the DSB, the wavelength of the emitted light could be tuned over a range of 100 nm. The syntheses of 6b—h were performed by twofold Wittig Horner-olefinations of bisphoshonates 1a, b with substituted benzaldehydes 2a—i, 6ivia Heck-reaction of the dibromosulfonylbenzene 3, 6k by Siegrist-reaction of 4 with N-phenylbenzaldimine and the Knoevenagel-reaction of benzyl cyanide with 5 led to 6l.

chemistry.chemical_compoundWavelengthUltraviolet visible spectroscopyChemistrylawWittig reactionBenzyl cyanideAbsorption (electromagnetic radiation)PhotochemistryFluorescence spectroscopySpectral lineLight-emitting diodelaw.inventionJournal für praktische Chemie
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Pyrene-fused bisphenazinothiadiazoles with red to NIR electroluminescence

2017

The synthesis and characterisation of two pyrene-fused phenazinothiadiazole derivatives with different substituents is described. Light-emitting diodes incorporating such derivatives display red to near-infrared electroluminescence with emission peaks at wavelengths as long as 721 nm, illustrating that pyrene-fused bisphenazinothiadiazoles can serve as deep red and NIR emitters.

chemistry.chemical_compoundWavelengthchemistry010405 organic chemistryOrganic ChemistryAnalytical chemistryPyreneElectroluminescence010402 general chemistryPhotochemistry01 natural sciences0104 chemical sciencesDiodeOrganic Chemistry Frontiers
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On the intrinsic population of the lowest triplet state of uracil

2007

Abstract From CASPT2//CASSCF quantum-chemical computations it is determined that the lowest triplet state of uracil can be efficiently populated from the initially activated singlet manifold through respective singlet–triplet crossings of the singlet state with the low-lying 3nπ∗ state at 4.6 eV and with the lowest 3ππ∗ state at 4.2 eV located along the minimum energy path of the low-lying 1ππ∗ state. Large spin–orbit coupling elements predict, in particular for the former case, efficient intersystem crossing processes. The wavelength dependence measured for the triplet quantum yield can be explained by the location of the singlet–triplet crossing regions.

education.field_of_studyChemistryPopulationGeneral Physics and AstronomyQuantum yieldState (functional analysis)WavelengthIntersystem crossingSinglet fissionSinglet statePhysical and Theoretical ChemistryAtomic physicsTriplet stateeducationChemical Physics Letters
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Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

2017

Astronomy and astrophysics 603, A31 (2017). doi:10.1051/0004-6361/201629540

extragalactic background lightmultiwavelength observationsAstrophysics::High Energy Astrophysical Phenomenabl-lacertae objectsGalaxies: BL Lacertae objects: individual: Markarian 501 ; Methods: data analysis ; observational ; Polarizationspectral energy-distributionFluxFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionindividual: Markarian 501 [BL Lacertae objects]lawCoincident0103 physical sciencesddc:530MAGIC (telescope)crab-nebulaBlazardata analysis [Methods]010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)tev blazars010308 nuclear & particles physicsstochastic accelerationtelescope observationsInstitut für Physik und AstronomieAstronomy and AstrophysicsAstronomy and Astrophysicgamma-ray emissionmethods: data analysis520BL Lacertae objects: individual: Markarian 501; Methods: data analysisSynchrotrondata analysi [Methods]BL Lacertae objects: individual: Markarian 501; Methods: data analysis; Astronomy and Astrophysics; Space and Planetary ScienceBL Lacertae objects: individual: Markarian 501x-raySpace and Planetary Scienceddc:520ElectrónicaFísica nuclearElectricidadDegeneracy (mathematics)Astrophysics - High Energy Astrophysical PhenomenaFlareBL Lac object
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Cladding-Pumped Er/Yb-Co-Doped Fiber Amplifier for Multi-Channel Operation

2022

The Institute of Solid State Physics, University of Latvia, as a Center of Excellence, has received funding from the European Union’s Horizon 2020 Framework Programme H2020-WIDESPREAD-01-2016-2017-TeamingPhase2 under grant agreement No. 739508, project CAMART2. We express our gratitude to rer. nat. Nicoletta Haarlammert from Fraunhofer Institute for Applied Optics and Precision Engineering IOF for the refractive index measurements of ytterbium/erbium-co-doped fibers. This work is supported by the European Regional Development Fund project No. 1.1.1.1/18/A/068.

fiber-optic systemsabsorption and emission spectra:NATURAL SCIENCES::Physics [Research Subject Categories]overlap factorRadiology Nuclear Medicine and imagingerbium/ ytterbium co-dopingwavelength division multiplexingInstrumentationcladding-pumped doped fiber amplifierAtomic and Molecular Physics and Opticsabsorption and emission spectra; cladding-pumped doped fiber amplifier; erbium/ytterbium co-doping; fiber-optic systems; overlap factor; wavelength division multiplexingPhotonics
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Dynamic SEDs of southern blazars - DSSB

2016

The Dynamic SEDs of southern blazars catalog is based on a TANAMI multiwavelength project that has been monitoring a sample of 22 radio-loud blazars of the southern sky from radio to gamma-ray wavelengths. (4 data files). Simultaneous broadband spectral and temporal studies of blazars are an important tool for investigating active galactic nuclei (AGN) jet physics. Aims. We study the spectral evolution between quiescent and flaring periods of 22 radio-loud AGN through multiepoch, quasi-simultaneous broadband spectra. For many of these sources these are the first broadband studies. Methods. We use a Bayesian block analysis of Fermi/LAT light curves to determine time ranges of constant flux f…

galactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsradio-loud blazarsAstrophysics::Cosmology and Extragalactic AstrophysicsSEDstellar astronomyMultiwavelengthobservational astronomyBL Lacertae objectsNatural SciencesQuasarsAstrophysics::Galaxy AstrophysicsSpectral energy distribution
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Longer wavelengths of light improve the growth, intake and feed efficiency of individually reared juvenile pikeperchSander lucioperca(L.)

2009

We tested the effects of monochromatic light on the specific growth rate (SGR), feed intake and feed efficiency (FE) of juvenile pikeperch, Sander lucioperca (L.). Pikeperch were reared individually for 42 days in aquaria covered with blue, green, yellow or red gelatin filters or white paper (control; n=5). Linear regression analysis indicated a significant positive effect of longer wavelengths of light on the condition factor (CF), FE and SGR. The final weight, SGR and CF were significantly higher in fish reared under red than under white light, and FE was better under green, yellow and red light than under white light (Dunnett's post hoc test, P<0.05) while blue was comparable to white li…

genetic structuresEcologyAquatic ScienceBiologyFeed conversion ratioVisual sensitivityCondition factorPigmentWavelengthAnimal scienceSpectral sensitivityvisual_artvisual_art.visual_art_mediumWhite lightJuvenilesense organsAquaculture Research
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En-Face differential absorption optical coherence tomography with gold nanorods as the contrast agent

2008

A new variety of nanoparticles showing unique and characteristic optical properties, appeals for its use as contrast agents in medical imaging. Gold nanospheres, nanorods and nanoshells with a silica core are new forms of promising contrast agents which can be tuned to specific absorption or scattering characteristics within the near-infrared (NIR) spectrum ranging from 650 - 1300 nm. They have the ability to be used for both image enhancement and as photosensitive markers due to their well designable scattering and absorption properties. Furthermore, their strong optical absorption permits treatment of malignant cells by photoablation processes, induced when heating them with a matched lig…

genetic structuresmedicine.diagnostic_testChemistryScatteringbusiness.industryNear-infrared spectroscopyPhotoablationNanoshellWavelengthOpticsOptical coherence tomographymedicineNanorodsense organsAbsorption (electromagnetic radiation)business1st Canterbury Workshop on Optical Coherence Tomography and Adaptive Optics
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Spotlight on fundus autofluorescence

2018

Ana M Calvo-Maroto,1 Alejandro Cervi&ntilde;o2 1Department of Ophthalmology, Cl&iacute;nica Universidad de Navarra, University of Navarra, Madrid, Spain; 2Optometry Research Group, Department of Optics and Optometry and Vision Sciences, University of Valencia, Valencia, Spain Abstract: Fundus autofluorescence (FAF) imaging is based on the fluorescence from ocular endogenous fluorophores located in the retinal pigment epithelium and choroid, mainly lipofuscin and melanin. It is a noninvasive technique that provides information about the spatial distribution of lipofuscin/melanin and retinal pigment epithelium health status. An overview about the fluorophores responsible for FAF imaging and t…

genetic structuresnear infrared fundus autofluorescence (NIR-FAF)lcsh:Ophthalmologylcsh:RE1-994sense organslipofuscinmelanin.eye diseasesFundus autofluorescenceshort wavelength fundus autofluorescence (SW-FAF)Clinical Optometry
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An X-ray characterization of the central region of the supernova remnant G332.5-5.6

2015

Aims. We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 through an exhaustive analysis of XMM-Netwon observations with complementary infrared observations. We characterize and discuss the origin of the observed X-ray morphology, which presents a peculiar plane edge over the west side of the central region. Methods. The morphology and spectral properties of the X-ray SNR were studied using a single full frame XMM-Netwon observation in the 0.3 to 10.0 keV energy band. Archival infrared WISE observations at 8, 12 and 24 μm were also used to investigate the properties of the source and its surroundings at different wavelengths. Results. The results show th…

individual objects: G332.5-5.6 [ISM]Ciencias AstronómicasISM: individual objects: G332.5-5.6InfraredSupernova remnantsCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRadiation//purl.org/becyt/ford/1 [https]Interstellar mediumIonizationX-raysRadiation mechanismsISM [X-rays]Supernova remnantCiencias Exactas y NaturalesAstrophysics::Galaxy AstrophysicsG332.5-5.6 (ISM individual objects)ISM: supernova remnantsPhysicssupernova remnants [ISM]Atomic emission spectroscopyAstronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]Thermal mechanismsRadiation mechanisms: thermalX-rays: ISMInterstellar mediumISM: individual objects: G332.5-5.6 ISM: supernova remnants X-rays: ISM radiation mechanisms: thermalAstronomíaWavelengthSpace and Planetary Sciencethermal [Radiation mechanisms]CIENCIAS NATURALES Y EXACTAS
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