Search results for "Rays"

showing 10 items of 1136 documents

Primary mouse fibroblasts deficient for c-Fos, p53 or for both proteins are hypersensitive to UV light and alkylating agent-induced chromosomal break…

2000

The important regulatory proteins, c-Fos and p53 are induced by exposure of cells to a variety of DNA damaging agents. To investigate their role in cellular defense against genotoxic compounds, we comparatively analysed chromosomal aberrations and apoptosis induced by ultraviolet (UV-C) light and the potent alkylating agent methyl methanesulfonate (MMS) in primary diploid mouse fibroblasts knockout for either c-Fos or p53, or double knockout for both genes. We show that c-Fos and p53 deficient fibroblasts are more sensitive than the corresponding wild-type cells as to the induction of chromosomal aberrations and apoptosis. Double knockout fibroblasts lacking both c-Fos and p53 are viable an…

Alkylating AgentsUltraviolet RaysDNA repairDNA damageHealth Toxicology and MutagenesisDrug ResistanceMutagenesis (molecular biology technique)ApoptosisBiologyRadiation ToleranceCell LineMicechemistry.chemical_compoundGeneticsAnimalsMolecular BiologyGene knockoutChromosome AberrationsMice KnockoutGenes fosFibroblastsCell cycleGenes p53Molecular biologyMethyl methanesulfonatechemistryApoptosisCell cultureTumor Suppressor Protein p53Proto-Oncogene Proteins c-fosDNA DamageMutation Research/Fundamental and Molecular Mechanisms of Mutagenesis
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Multioctave midinfrared supercontinuum generation in suspended-core chalcogenide fibers

2014

An As2S3 fiber-based supercontinuum source that covers 3500 nm, extending from near visible to the midinfrared, is successfully reported by using a 200-fs-pulsed pump with nJ-level energy at 2.5 μm. The main features of our fiber-based source are two-fold. On the one hand, a low-loss As2S3 microstructured optical fiber has been fabricated, with typical attenuation below 2 dB/m in the 1-4 μm wavelength range. On the other hand, a 20-mm-long microstructured fiber sample is sufficient to enable a spectral broadening, spreading from 0.6 to 4.1 μm in a 40 dB dynamic range.

All-silica fiberPHOSFOSMaterials scienceInfrared Raysbusiness.industryEquipment DesignMicrostructured optical fiberSulfidesArsenicalsAtomic and Molecular Physics and OpticsSupercontinuumEquipment Failure AnalysisOpticsZero-dispersion wavelengthEnergy TransferChalcogensOptoelectronicsDispersion-shifted fiberbusinessPlastic optical fiberOptical FibersPhotonic-crystal fiberOptics Letters
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Microstructured chalcogenide optical fibers from As2S3 glass: towards new IR broadband sources

2010

Made available in DSpace on 2013-08-28T14:12:29Z (GMT). No. of bitstreams: 1 WOS000285749500124.pdf: 1017839 bytes, checksum: f517fd8ef33fd56d66b9ccda9dc4d0f3 (MD5) Made available in DSpace on 2013-09-30T19:22:53Z (GMT). No. of bitstreams: 2 WOS000285749500124.pdf: 1017839 bytes, checksum: f517fd8ef33fd56d66b9ccda9dc4d0f3 (MD5) WOS000285749500124.pdf.txt: 33157 bytes, checksum: 1ca2ac713bf6024674249abf58520bcb (MD5) Previous issue date: 2010-12-06 Submitted by Vitor Silverio Rodrigues (vitorsrodrigues@reitoria.unesp.br) on 2014-05-20T15:34:00Z No. of bitstreams: 2 WOS000285749500124.pdf: 1017839 bytes, checksum: f517fd8ef33fd56d66b9ccda9dc4d0f3 (MD5) WOS000285749500124.pdf.txt: 33157 bytes,…

All-silica fiberPHOSFOSOptical fiberMaterials scienceInfrared RaysChalcogenide glass02 engineering and technologySulfides01 natural sciencesArsenicalslaw.invention010309 opticsOpticsZero-dispersion wavelengthlaw0103 physical sciencesFiber Optic TechnologyLightingMiniaturizationbusiness.industryMicrostructured optical fiber[CHIM.MATE]Chemical Sciences/Material chemistryEquipment Design021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsEquipment Failure Analysis[ CHIM.MATE ] Chemical Sciences/Material chemistryChalcogensGlass0210 nano-technologybusinessHard-clad silica optical fiberPhotonic-crystal fiber
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EAACI Position paper on the standardization of nasal allergen challenges.

2018

DR. FARID, S.H. M.H. M. Kn. - FR FARID/0000-0003-0372-4963; Gevaert, Philippe/0000-0002-1629-8468; Hox, Valerie/0000-0003-2390-294X; Wagenman, Martin/0000-0002-9734-0241; Vent, Julia/0000-0001-5071-9580 WOS: 000438710600002 PubMed: 29377177 Nasal allergen challenge (NAC) is an important tool to diagnose allergic rhinitis. In daily clinical routine, experimentally, or when measuring therapeutic success clinically, nasal allergen challenge is fundamental. It is further one of the key diagnostic tools when initiating specific allergen immunotherapy. So far, national recommendations offered guidance on its execution; however, international divergence left many questions unanswered. These differ…

Allergen immunotherapymedicine.medical_specialtyNasal Provocation TestsStandardizationImmunologyAdvisory CommitteesAftercareallerginen nuhaDiagnostic toolsmedicine.disease_causeSneezingdiagnostic toolsUnmet needsAllergen challenge03 medical and health sciences0302 clinical medicineAllergennasal provocation testGermanyotorhinolaryngologic diseasesImmunology and AllergyMedicineHumans030223 otorhinolaryngologyIntensive care medicineAnaphylaxisAdministration IntranasalSkin TestsProtocol (science)allergic rhinitisbusiness.industryaltistuskoePruritusNasal Spraysrespiratory systemAllergensImmunoglobulin ERhinitis Allergicta3125Nasal Mucosa030228 respiratory systemPosition paperNasal Obstructionnasal allergen challengebusinessAllergy
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<title>Stereovision studies by disbalanced images</title>

2003

Studies are focused on design and appraisal of an objective test of the quality of stereovision depending on optical stimuli blurring and detecting of the stereovision threshold at various stimuli blur degree. The method is based on the principles of grayscale and color random dot stereotests. Experiments may be divided with respect to the principle of demonstration: 1) the blur is modeled by defocusing an optical lens - the strength of the optical system is varied at a constant quality of the stimulus, or 2) the blur is simulated on the computer screen - here the quality of the stimulus varies. To obtain an independent description and to measure blurring the experimentally demonstrated ima…

Amplitude modulationsymbols.namesakeFourier transformbusiness.industryStereotestssymbolsComputer visionArtificial intelligencebusinessGrayscaleComputing systemsMathematicsSPIE Proceedings
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Pressure-induced magnetic switching and linkage isomerism in K0.4Fe4[Cr(CN)6]2.8 x 16 H2O: X-ray absorption and magnetic circular dichroism studies.

2008

The effect of applied pressure on the magnetic properties of the Prussian blue analogue K0.4Fe4[Cr(CN)6]2.8 x 16 H2O (1) has been analyzed by dc and ac magnetic susceptibility measurements. Under ambient conditions, 1 orders ferromagnetically at a critical temperature (T(C)) of 18.5 K. Under application of pressure in the 0-1200 MPa range, the magnetization of the material decreases and its critical temperature shifts to lower temperatures, reaching T(C) = 7.5 K at 1200 MPa. Pressure-dependent Raman and Mossbauer spectroscopy measurements show that this striking behavior is due to the isomerization of some Cr(III)-C[triple bond]N-Fe(II) linkages to the Cr(III)-N[triple bond]C-Fe(II) form. A…

Analytical chemistryBiochemistryCatalysisMagnetizationsymbols.namesakeMagneticsColloid and Surface ChemistryIsomerismX-Ray DiffractionChromium CompoundsMössbauer spectroscopyTavernePressureLinkage isomerismCyanidesMagnetic circular dichroismChemistrySpectrum AnalysisX-RaysTemperatureWaterGeneral ChemistryMagnetic susceptibilityX-ray magnetic circular dichroismsymbolsDiamagnetismRaman spectroscopyCrystallizationIron CompoundsJournal of the American Chemical Society
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Receptor Activator of NF-kB (RANK) Expression in Primary Tumors Associates with Bone Metastasis Occurrence in Breast Cancer Patients

2011

Background\ud Receptor activator of NFkB (RANK), its ligand (RANKL) and the decoy receptor of RANKL (osteoprotegerin, OPG) play a pivotal role in bone remodeling by regulating osteoclasts formation and activity. RANKL stimulates migration of RANK-expressing tumor cells in vitro, conversely inhibited by OPG.\ud \ud Materials and Methods\ud We examined mRNA expression levels of RANKL/RANK/OPG in a publicly available microarray dataset of 295 primary breast cancer patients. We next analyzed RANK expression by immunohistochemistry in an independent series of 93 primary breast cancer specimens and investigated a possible association with clinicopathological parameters, bone recurrence and surviv…

Anatomy and PhysiologyMicroarraysSettore MED/06 - Oncologia MedicaCancer TreatmentLigandsMetastasisBone remodelingMetastasisBasic Cancer ResearchBreast TumorsBone and Soft Tissue SarcomasNeoplasm MetastasisMusculoskeletal SystemOligonucleotide Array Sequence AnalysisMultidisciplinaryPredictive markerReceptor Activator of Nuclear Factor-kappa BQRBone metastasisMiddle AgedImmunohistochemistryGene Expression Regulation NeoplasticOncologyRANKLMedicineFemaleResearch Articlemusculoskeletal diseasesmedicine.medical_specialtyHistologyScienceBone NeoplasmsBreast NeoplasmsBiologyBreast cancerAntibody TherapySDG 3 - Good Health and Well-beingOsteoprotegerinInternal medicinemedicineHumansRNA MessengerBoneBiologyAgedBreast cancer bone metastasis RANK-RANKLRANK LigandOsteoprotegerinComputational BiologyCancers and NeoplasmsRANK Ligandmedicine.diseaseEndocrinologyCancer researchbiology.protein
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A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

2010

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierr…

Angstrom exponentAstronomyAstrophysics01 natural sciencesAugerCROSS-SECTIONSCOSMIC-RAY SHOWERSObservatoryDEPENDENCEHigh-Energy Cosmic Ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Lidar[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ANGSTROM EXPONENTPierre Auger ObservatoryBi-static lidarELECTRONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMULTIPLE-SCATTERINGLight emissionFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLIGHT-EMISSIONAstrophysics - Cosmology and Nongalactic Astrophysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Extensive air showerFOS: Physical sciencesCosmic raySURFACE DETECTORAir fluorescence method0103 physical sciencesExtensive air showersRECONSTRUCTIONAerosolInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryAerosolsCalorimeter (particle physics)Atmospheric effect010308 nuclear & particles physicsAtmosphereFísicaAstronomy and AstrophysicsCosmic rays; Extensive air showers; Air fluorescence method; Atmosphere; Aerosols; Lidar; Bi-static lidarCosmic rayNITROGENAir showerFluorescence Telescopes13. Climate actionExperimental High Energy PhysicsAEROSSOL
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Neutrino pair annihilation near accreting, stellar-mass black holes

2006

We investigate the energy-momentum deposition due to neutrino-antineutrino annihilation in the vicinity of axisymmetric, accreting black holes (BHs) by numerically ray-tracing neutrino trajectories in a Kerr space-time. Hyperaccreting stellar-mass BHs are widely considered as energy sources that can drive ultrarelativistic outflows with the potential to produce gamma-ray bursts. In contrast to earlier works, we provide an extensive and detailed parameter study of the influence of general relativistic (GR) effects and of different neutrinosphere geometries. These include idealized thin disks, tori, and spheres, or are constructed as non-selfgravitating equilibrium matter distributions for va…

Angular momentumAccretionStellar massAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsNeutronUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsRelativityNeutrinosPhysicsBurstsAnnihilationAstrophysics (astro-ph)Gamma raysAstronomy and AstrophysicsTorusRadiusBlack hole physicsGamma rays ; Bursts ; Neutrinos ; Accretion ; Accretion disks ; Relativity ; Black hole physics ; Neutron:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceAccretion disksSPHERESUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaNeutrinoEnergy source:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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On the timing properties of SAX J1808.4-3658 during its 2015 outburst

2017

We present a timing analysis of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, using non-simultaneous XMM-Newton and NuStar observations. We estimate the pulsar spin frequency and update the system orbital solution. Combining the average spin frequency from the previous observed, we confirm the long-term spin down at an average rate $\dot{\nu}_{\text{SD}}=1.5(2)\times 10^{-15}$ Hz s$^{-1}$. We also discuss possible corrections to the spin down rate accounting for mass accretion onto the compact object when the system is X-ray active. Finally, combining the updated ephemerides with those of the previous outbursts, we find a long-term orbital evolution compatibl…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsCompact star01 natural sciencespulsars: individual: SAX J1808.4-3658Gravitationstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsar0103 physical sciences010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsOrbital periodaccretion accretion discs; stars: neutron; pulsars: individual: SAX J1808.4-3658; X-rays: binaries13. Climate actionSpace and Planetary ScienceQuadrupole:accretion accretion discAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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