Search results for "CIENCIAS NATURALES Y EXACTAS"

showing 10 items of 280 documents

Comparative survey of putrescine production from agmatine deamination in different bacteria

2008

This article aims to study putrescine production in Lactobacillus hilgardii strain X1B, an agmatine degrader isolated from wine, and to compare it with three other different species, previously reported as putrescine producers from agmatine: Pseudomonas aeruginosa PAO1, Enterococcus faecalis ATCC11700 and Bacillus cereus CECT 148T. The effect of different biogenic amines, organic acids, cofactors, amino acids and sugars on putrescine production was evaluated. In some cases, a similar effect was found in all the strains studied but the magnitude differed. Arginine, glucose and fructose showed an inhibitory effect, whereas the presence of agmatine induced the production of putrescine in all m…

Biogenic AminesAgmatineArginineOtras Ciencias Biológicasved/biology.organism_classification_rank.speciesSpermineWineLactobacillus hilgardiiBiologyArginineMicrobiologyEnterococcus faecalisCiencias Biológicaschemistry.chemical_compoundBacillus cereusSpecies SpecificityEnterococcus faecalisPutrescineved/biologyBIOGENIC AMINESWINEbiology.organism_classificationPUTRESCINESpermidineAgmatine deiminaseLactobacilluschemistryBiochemistryPseudomonas aeruginosaPutrescineAGMATINE DEIMINASEAgmatineCIENCIAS NATURALES Y EXACTASFood ScienceFood Microbiology
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Tucupentol, a novel mono-tetrahydrofuranic acetogenin from Annona montana, as a potent inhibitor of mitochondrial complex I.

2009

Ten acetogenins, one of them new, were isolated from leaves and twigs of a Bolivian collection of Annona montana. The new compound that we named tucupentol (1) is a mono-tetrahydrofuranpentahydroxy-acetogenin. The inhibitory potency of tucupentol (1) on the mitochondrial complex I was evaluated, and this activity was compared with that of the known acetogenins, annonacin-A, cisannonacin-10-one, aromin, and gigantetronenin, also isolated from this plant material. The mentioned acetogenins acted as selective inhibitors of mitochondrial complex I in the 0.8-5.4-nM range. Fil: Álvarez Colom, Olga. Universidad Nacional de Tucumán. Facultad de Bioquímica, Química y Farmacia. Instituto de Química …

BoliviaAcetogeninsBioengineeringGigantetroneninMitochondrionBiochemistryAnnonaMitochondria Heartchemistry.chemical_compoundInhibitory Concentration 50AnimalsMedicinal plantsFuransMolecular BiologyNuclear Magnetic Resonance BiomolecularTucupentolElectron Transport Complex IbiologyPlant StemsOtras Ciencias QuímicasCiencias QuímicasGeneral ChemistryGeneral Medicinebiology.organism_classificationAnnona montanaPlant LeavesInhibitory potencychemistryBiochemistryAcetogeninMolecular MedicineCattleCIENCIAS NATURALES Y EXACTASMitochondrial Complex IChemistrybiodiversity
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Tailoring the Exchange Interaction in Covalently Linked Basic Carboxylate Clusters through Bridging Ligand Selection

2012

We are reporting new dimeric units of basic carboxylates bearing the {Fe III 2M IIO} motif for M = Co and Ni, covalently bound through the tetradentate bridging (LL) 2,2′-azopyiridine (azpy) and 2,3-di(2-pyridyl)quinoxaline ligands (dpq). We structurally characterized the hexanuclear clusters, and their magnetic properties have been fully analyzed. DFT calculations have been performed as a supplementary tool. All results evidence a weak antiferromagnetic interaction through the bridging ligands between isolated spin ground states arising from intra-Fe 2MO core exchange couplings. Together with the pioneer 2,2′-bipyrimidine bridged systems, the new complexes reported constitute a family of c…

Bridging (networking)LigandStereochemistryOtras Ciencias QuímicasExchange interactionCiencias QuímicasQUANTUM INFORMATIONBridging ligandSINGLE-MOLECULE MAGNETS//purl.org/becyt/ford/1 [https]Inorganic Chemistrychemistry.chemical_compoundQuinoxalinechemistryGROUND SPIN-STATECovalent bond//purl.org/becyt/ford/1.4 [https]AntiferromagnetismCarboxylatePIVALATE COMPLEXESPhysical and Theoretical ChemistryCIENCIAS NATURALES Y EXACTASInorganic Chemistry
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Defense Responses in Two Ecotypes of Lotus japonicus against Non-Pathogenic Pseudomonas syringae

2013

Lotus japonicus is a model legume broadly used to study many important processes as nitrogen fixing nodule formation and adaptation to salt stress. However, no studies on the defense responses occurring in this species against invading microorganisms have been carried out at the present. Understanding how this model plant protects itself against pathogens will certainly help to develop more tolerant cultivars in economically important Lotus species as well as in other legumes. In order to uncover the most important defense mechanisms activated upon bacterial attack, we explored in this work the main responses occurring in the phenotypically contrasting ecotypes MG-20 and Gifu B-129 of L. ja…

CIENCIAS MÉDICAS Y DE LA SALUDSTRESSLotus japonicusLotusInmunologíaDefence mechanismslcsh:MedicinePseudomonas syringaePlant disease resistanceCiencias BiológicasSYRINGAE//purl.org/becyt/ford/1 [https]Gene Expression Regulation PlantTRANSCRIPTOMICBotanyPseudomonas syringaePlant defense against herbivoryArabidopsis thalianalcsh:Science//purl.org/becyt/ford/1.6 [https]Ciencias de las Plantas BotánicaDisease ResistanceOligonucleotide Array Sequence AnalysisPlant DiseasesEcotypeMultidisciplinarybiologyEcotypeLOTUSGene Expression Profilinglcsh:Rfungifood and beverages//purl.org/becyt/ford/3.1 [https]biology.organism_classificationBIOTICMedicina BásicaJAPONICUSLotuslcsh:Q//purl.org/becyt/ford/3 [https]PSEUDOMONASCIENCIAS NATURALES Y EXACTASResearch ArticlePLoS ONE
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Geochemical evidence for arsenic cycling in living microbialites of a High Altitude Andean Lake (Laguna Diamante, Argentina)

2020

Arsenic is best known as an environmental toxin, but this element could also serve as a metabolic energy source to certain microorganisms. Moreover, As cycling may have driven microbial life on early Earth prior to oxygenation of the atmosphere. Still, little is known about the arsenic cycling processes occurring in the presence of microorganisms and the possible traces that could be preserved in the rock record. To advance our understanding of this we studied the geochemical proxies of microbial As metabolism in living microbialites from Laguna Diamante, a likely Precambrian ecosystem analogue (Catamarca, Argentina). In this study, we show that the coexistence of As(III) and As(V) strongly…

Carbonate010504 meteorology & atmospheric sciencesSynchrotron-based X-ray imagingchemistry.chemical_element010502 geochemistry & geophysicsGeologic record01 natural sciencesEarly lifechemistry.chemical_compoundPrecambrian[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryANDES LAKESGeochemistry and PetrologyExtremophileEcosystemArsenic cyclingArsenic0105 earth and related environmental sciencesEXTREMOPHILEEcologyMicrobialitesOtras Ciencias Naturales y ExactasGeologyARCHEAEEarly Earthchemistry13. Climate actionCarbonateCalciumARSENICCyclingCIENCIAS NATURALES Y EXACTASGeologyChemical Geology
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Photoactivation of Anticancer Ru Complexes in Deep Tissue: How Deep Can We Go?

2017

Activation of anticancer therapeutics such as ruthenium (Ru) complexes is currently a topic of intense investigation. The success of phototherapy relies on photoactivation of therapeutics after the light passes through skin and tissue. In this paper, the photoactivation of anticancer Ru complexes with 671-nm red light through tissue of different thicknesses was studied. Four photoactivatable Ru complexes with different absorption wavelengths were synthesized. Two of them (Ru3 and Ru4) were responsive to wavelengths in the “therapeutic window” (650–900 nm) and could be activated using 671-nm red light after passing through tissue up to 16-mm-thick. The other two (Ru1 and Ru2) could not be ac…

Cell SurvivalInfrared Rayschemistry.chemical_elementAntineoplastic Agents02 engineering and technologyAbsorption (skin)010402 general chemistryPhotochemistry01 natural sciencesCatalysisRutheniumMETALLODRUGDeep tissueCoordination ComplexesHumansRed lightPHOTOTHERAPYTherapeutic windowChemistryPHOTOCHEMISTRYOtras Ciencias QuímicasOrganic ChemistryLight activatedCiencias QuímicasGeneral Chemistry021001 nanoscience & nanotechnology0104 chemical sciencesRutheniumRU COMPLEXSpectrophotometryCancer cellANTICANCER0210 nano-technologyCIENCIAS NATURALES Y EXACTASHeLa Cells
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Rational design of covalently bridged [FeIII2MIIO] clusters

2010

We are reporting the first supramolecular dimeric units of basic carboxylates. The neutral [FeIII 2MIIO] motif for different 3d M metals is covalently bound through 2,2′-bipyrimidine. We have structurally characterized the hexanuclear clusters and the related trinuclear building blocks. Their magnetic properties have been fully analyzed and DFT calculations have been performed as a supplementary tool. All results evidence a weak antiferromagnetic interaction through the bpym bridge between isolated spin ground states (in some examples) arising from intra-Fe 2MO core exchange couplings. Fil: Alborés, Pablo. Johannes Gutenberg Universitat Mainz; Alemania. Consejo Nacional de Investigaciones C…

ChemistryOtras Ciencias Químicasbasic carboxylateCiencias QuímicasRational designSupramolecular chemistrybipyrimidineInorganic Chemistrycovalently linkComputational chemistryCovalent bondAntiferromagnetismmagnetic propertiesSpin (physics)CIENCIAS NATURALES Y EXACTASDalton Transactions
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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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