Search results for "RAYS"

showing 10 items of 1136 documents

Aggregation versus Biological Activity in Gold(I) Complexes. An Unexplored Concept

2021

The aggregation process of a series of mono- and dinuclear gold(I) complexes containing a 4-ethynylaniline ligand and a phosphane at the second coordination position (PR3-Au-C≡CC6H4-NH2, complexes 1-5, and (diphos)(Au-C≡CC6H4-NH2)2, complexes 6-8), whose biological activity was previously studied by us, has been carefully analyzed through absorption, emission, and NMR spectroscopy, together with dynamic light scattering and small-angle X-ray scattering. These experiments allow us to retrieve information about how the compounds enter the cells. It was observed that all compounds present aggregation in fresh solutions, before biological treatment, and thus they must be entering the cells as a…

ChemistryLigandScatteringBiological activityOrNuclear magnetic resonance spectroscopyAggregation (Chemistry)Inorganic ChemistryCrystallographyDynamic light scatteringAgregació (Química)X-raysRaigs XGoldPhysical and Theoretical ChemistryAbsorption (chemistry)Inductively coupled plasmaCytoskeletonCytoskeleton
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Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

2023

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy $\gamma$-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs whi…

Cherenkov Telescope ArrayGamma rays: generalstatistical [methods]energy spectrumFOS: Physical sciencesVHESettore FIS/05 - Astronomia E Astrofisicacosmic raysMethods: data analysissupernovadata analysis [methods][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov Telescope Arra ; alactic Supernova Remnants ; PeVatrons ;Methods: statisticalgalactic PeVatronsHigh Energy Astrophysical Phenomena (astro-ph.HE)emission spectrum) supernovae: general [(stars]Astronomy and AstrophysicssensitivityobservatoryGalactic PeVatronscosmic radiationspectralgalaxyhadron(Stars:) supernovae: generalAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalgeneral [gamma rays]signature
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Spectral attenuation of solar ultraviolet radiation in humic lakes in Central Finland

2003

The attenuation of solar ultraviolet (UV) radiation in five lakes in Central Finland was evaluated through field measurements and/or by determining the optical properties of the lake water during summer 1999. Spectral UV irradiance in the air and at several depths underwater was measured in three lakes (Lake Palosjärvi, Konnevesi, and Jyväsjärvi) with dissolved organic carbon (DOC) ranging from 4.9 to 8.7 mg l(-1) and chlorophyll a ranging from 1.6 to 16 g l(-1). According to the field measurements, 99% of the UV-B radiation was attenuated in approximately a half meter water column in the clearest lake. In the UV-A region at 380 nm, the corresponding attenuation occurred in the upper one me…

ChlorophyllChlorophyll aEnvironmental EngineeringUltraviolet RaysHealth Toxicology and MutagenesisIrradianceFresh WaterRadiationmedicine.disease_causeAbsorptionchemistry.chemical_compoundWater columnDissolved organic carbonmedicineEnvironmental ChemistryFinlandAttenuationPublic Health Environmental and Occupational HealthGeneral MedicineGeneral ChemistryPollutionchemistryEnvironmental chemistryAttenuation coefficientEnvironmental scienceUltravioletChemosphere
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Response to long-term NaHCO3-derived alkalinity in model Lotus japonicus Ecotypes Gifu B-129 and Miyakojima MG-20: transcriptomic profiling and physi…

2014

The current knowledge regarding transcriptomic changes induced by alkalinity on plants is scarce and limited to studieswhere plants were subjected to the alkaline salt for periods not longer than 48 h, so there is no information availableregarding the regulation of genes involved in the generation of a new homeostatic cellular condition after long-termalkaline stress.Lotus japonicusis a model legume broadly used to study many important physiological processes includingbiotic interactions and biotic and abiotic stresses. In the present study, we characterized phenotipically the response toalkaline stress of the most widely usedL. japonicusecotypes, Gifu B-129 and MG-20, and analyzed global t…

ChlorophyllOtras Biotecnología AgropecuariaPhysiologyApplied MicrobiologyPlant SciencePathogenesisPathology and Laboratory MedicinePlant RootsBiochemistryTranscriptomeZINCchemistry.chemical_compoundPlant MicrobiologyGene Expression Regulation PlantABIOTIC STRESSMETAL TRANSPORTERSMedicine and Health SciencesOligonucleotide Array Sequence AnalysisLOTUS JAPONICUSPlant Growth and DevelopmentMultidisciplinarybiologyEcotypePlant BiochemistryIRONQRMicrobial Growth and Development//purl.org/becyt/ford/4.4 [https]food and beveragesPlantsZincPlant PhysiologyShootHost-Pathogen InteractionsMedicineAntacidsAnatomymicroarrayPlant ShootsResearch ArticleBiotechnologyHistologyScienceIronPlant Cell BiologyLotus japonicusBiotecnología AgropecuariaalkalinityMycologyReal-Time Polymerase Chain ReactionResearch and Analysis MethodsMicrobiologyModel OrganismsIsoflavonoidSpecies SpecificityPlant and Algal ModelsBotanyAbiotic stressGene Expression ProfilingfungiOrganismsFungiBiology and Life SciencesPlant TranspirationCell Biologybiology.organism_classificationMICROARRAYSGene expression profilingSodium BicarbonatechemistryCIENCIAS AGRÍCOLASChlorophyllLotusPhysiological Processes//purl.org/becyt/ford/4 [https]Developmental BiologyPloS one
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TFIIH Operates through an Expanded Proximal Promoter To Fine-Tune c-myc Expression

2004

A continuous stream of activating and repressing signals is processed by the transcription complex paused at the promoter of the c-myc proto-oncogene. The general transcription factor IIH (TFIIH) is held at promoters prior to promoter escape and so is well situated to channel the input of activators and repressors to modulate c-myc expression. We have compared cells expressing only a mutated p89 (xeroderma pigmentosum complementation group B [XPB]), the largest TFIIH subunit, with the same cells functionally complemented with the wild-type protein (XPB/wt-p89). Here, we show structural, compositional, and functional differences in transcription complexes between XPB and XPB/wt-89 cells at t…

Chromatin ImmunoprecipitationDNA ComplementaryCell SurvivalUltraviolet RaysBlotting WesternGreen Fluorescent ProteinsGene ExpressionRepressorCellular homeostasisBiologyTransfectionModels BiologicalProto-Oncogene MasProto-Oncogene Proteins c-mycTranscription Factors TFIIRibonucleasesPotassium PermanganateTranscription (biology)HumansRNA MessengerPromoter Regions GeneticMolecular BiologyModels GeneticGeneral transcription factorCell CycleGenetic Complementation TestDNA HelicasesPromoterCell BiologyFibroblastsFlow CytometryMolecular biologyDNA-Binding ProteinsKineticsTranscription Factor TFIIHMicroscopy FluorescenceMutationTranscription preinitiation complexTranscription factor II HTranscription Factor TFIIHPlasmidsMolecular and Cellular Biology
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Biogenic synthesis of palladium nanoparticles using Pulicaria glutinosa extract and their catalytic activity towards the Suzuki coupling reaction.

2014

Green synthesis of nanomaterials finds the edge over chemical methods due to its environmental compatibility. Herein, we report a facile and eco-friendly method for the synthesis of palladium (Pd) nanoparticles (NPs) using an aqueous solution of Pulicaria glutinosa, a plant widely found in a large region of Saudi Arabia, as a bioreductant. The as-prepared Pd NPs were characterized using ultraviolet-visible (UV-vis) spectroscopy, powder X-ray diffraction (XRD), transmission electron microscopy (TEM), energy-dispersive X-ray spectroscopy (EDX), and Fourier transform-infrared spectroscopy (FT-IR). The hydroxyl groups of the plant extract (PE) molecules were found mainly responsible for the red…

Chromatography GasMagnetic Resonance SpectroscopyStereochemistrychemistry.chemical_elementNanoparticleLigandsCatalysisCatalysisNanomaterialsPulicariaInorganic ChemistrySuzuki reactionMicroscopy Electron TransmissionX-Ray DiffractionSpectroscopy Fourier Transform InfraredMoleculeAqueous solutionChemistryPlant ExtractsX-RaysTemperatureGreen Chemistry TechnologyTransmission electron microscopyNanoparticlesSpectrophotometry UltravioletPalladiumNuclear chemistryPalladiumBromobenzenesDalton transactions (Cambridge, England : 2003)
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Detailed study of SNR G306.3–0.9 using XMM-Newton and Chandra observations

2016

Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant (SNR) G306.3-0.9 in detail to obtain constraints on its ionization stage, the progenitor supernova explosion, and the age of the remnant. Methods. We used combined data from XMM-Newton and Chandra observatories to study the X-ray morphology of G306.3-0.9 in detail. A spatially resolved spectral analysis was used to obtain physical and geometrical parameters of different regions of the remnant. Spitzer infrared observations, available in the archive, were also used to constrain the progenitor supernova and study the environment in which the remnant evol…

Ciencias AstronómicasInfraredCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaISM [Infrared]FOS: Physical sciencesthermal [radiation mechanism]individual objects: SNR G306.3–0.9 [ISM]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral line//purl.org/becyt/ford/1 [https]ISM: individual objects: SNR G306.3IonizationISM [X-ray]0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsISM [X-rays]Radio continuum: ISMEjectaSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Infrared: ISM010308 nuclear & particles physicssupernova remnants [ISM]Astronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]Astronomy and AstrophysicISM: individual objects: SNR G306.3–0.9ISM [Radio continuum]Radiation mechanisms: thermalX-rays: ISMindividual objects: G306.3-0.9 [ISM]Interstellar mediumAstronomíaSupernovathermal [Radiation mechanisms]Space and Planetary ScienceISM; ISM: individual objects: SNR G306.3; ISM: supernova remnants; Radiation mechanisms: thermal; Radio continuum: ISM; X-rays: ISM; Astronomy and Astrophysics; Space and Planetary Science [0.9; Infrared]0.9Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory an…

2014

Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant devia…

Ciencias FísicasAstronomyRaysAstrophysicsAstroparticle physics; Cosmic rays01 natural scienceslaw.inventionPierrelawAnisotropyTelescope010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]Energy[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicRadiación cósmicaAugerCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsCIENCIAS NATURALES Y EXACTASHigh[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raySURFACE DETECTORICECUBETelescopeAIR-SHOWER ARRAYDirectionscosmic rays0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsArraySpectral densitySpherical harmonicsFísicaAstronomy and AstrophysicsASTROFÍSICAUltra[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaDipoleRESOLUTIONSpace and Planetary ScienceExperimental High Energy PhysicsQuadrupoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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SHOCK-CLOUD INTERACTION AND PARTICLE ACCELERATION IN THE SOUTHWESTERN LIMB OF SN 1006

2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relatively tenuous and uniform environment despite interacting with an atomic cloud in its northwestern limb. The X-ray image of SN 1006 reveals an indentation in the southwestern part of the shock front and the H I maps show an isolated (southwestern) cloud, having the same velocity as the northwestern cloud, whose morphology fits perfectly in the indentation. We performed spatially resolved spectral analysis of a set of small regions in the southwestern nonthermal limb and studied the deep X-ray spectra obtained within the XMM-Newton SN 1006 Large Program. We also analyzed archive H I data, obtain…

Ciencias FísicasAstrophysics::High Energy Astrophysical PhenomenaHadronSynchrotron radiationAstrophysicsSpectral lineISM: cloudIndentationSupernova remnantISM: individual objects (SN 1006)acceleration of particleISM: supernova remnantAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicssupernova remnants X-rays: ISM [ISM]Astronomy and AstrophysicsX-rays: ISMShock (mechanics)Particle accelerationAstronomíaSpace and Planetary Scienceindividual objects: SN 1006 [ISM]clouds [ISM]CIENCIAS NATURALES Y EXACTASFermi Gamma-ray Space Telescope
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