Search results for "NGAL"

showing 10 items of 1796 documents

Energy transfer to xanthene dyes in dansylated POPAM dendrimers

2011

Abstract Excitation energy transfer (EET) in host–guest complexes of dansylated POPAM dendrimers and xanthene dyes have been studied by transient absorption spectroscopy. EET from dansyl periphery to guests: rose bengal, eosin, or fluorescein, showed non-exponential behaviour as a result of distribution of donor–acceptor distances. Time constants range from 100 fs to 8 ps, independent of the dye and the dendrimer generation. Experiments suggested that in dendrimers binding more than one guest, EET among the guests becomes effective. Guest–host and guest–guest interactions induce non-radiative relaxation channels making excitation decays of the guests clearly faster in complexes than in solu…

XantheneEosinRelaxation (NMR)General Physics and AstronomyPhotochemistrychemistry.chemical_compoundchemistryDendrimerUltrafast laser spectroscopyRose bengalPhysical and Theoretical ChemistrySpectroscopyta116ExcitationChemical Physics Letters
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First Dark Matter Search Results from the XENON1T Experiment

2017

We report the first dark matter search results from XENON1T, a ∼2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)-kg fiducial mass and in the [5,40] keVnr energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10-4 events/(kg×day×keVee), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consisten…

Xenon[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Massive particleGeneral Physics and Astronomy01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)RecoilXenonWIMPS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]PhysicsRange (particle radiation)Time projection chamberDetectorHigh Energy Physics - Phenomenologydark matter: scatteringTPCAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPDark matterFOS: Physical scienceschemistry.chemical_elementWIMP: massS030DI2Nuclear physicsPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesrecoil[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physique010308 nuclear & particles physicsbackgrounddark matter: detectorAstronomieGran SassochemistryDirect Searchtime projection chamber: xenoninterpretation of experiments: XENON[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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The universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample

2018

The hot plasma in galaxy clusters is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode information on the processes leading to the thermalization of the gas in the cluster's potential well as well as non-gravitational processes such as gas cooling, AGN feedback and kinetic energy. In this work we present the radial profiles of the thermodynamic properties of the intracluster medium (ICM) out to the virial radius for a sample of 12 galaxy clusters selected from the Planck all-sky survey. We determine the universal profiles of gas density, temperature, pressure, and entropy over more than two decades in radius…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector

2010

A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured lightest Kaluza-Klein particle (LKP) WIMPs in the Sun and converted to limits on the LKP-proton cross-sections for LKP masses in the range 250 -- 3000 GeV. These results are the most stringent limits to date on LKP annihilation in the Sun.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsSolar neutrinoDark matterFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesDark matterddc:530010306 general physicsCosmic raysHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAnnihilationMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Massless particleNeutrino detectorHigh Energy Physics::ExperimentOther gauge bosonsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonPhysical Review D
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The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

2019

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unveil the composition and dynamics of the faint Universe and impact nearly every field of astrophysics across all spatial scales, from individual stars to the largest scale structures in the Universe. Major pillars in the science program for MSE include (i) the ultimate Gaia follow-up facility for understanding the chemistry and dynamics of the distant Milky Way, including the outer disk and faint stellar halo at high spectral resolution (ii) galaxy formation and evolution at cosmic noon, via the type of revolutionary…

[PHYS]Physics [physics]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies[PHYS] Physics [physics][SDU] Sciences of the Universe [physics][SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Monitoring of atrazine treatment on soil bacterial, fungal and atrazine-degrading communities by quantitative competitive PCR

2003

We report the development of quantitative competitive (QC) PCR assays for quantifying the 16S, 18S ribosomal and atzC genes in nucleic acids directly extracted from soil. QC-PCR assays were standardised, calibrated and evaluated with an experimental study aiming to evaluate the impact of atrazine application on soil microflora. Comparison of QC-PCR 16S and 18S results with those of soil microbial biomass showed that, following atrazine application, the microbial biomass was not affected and that the amount of 16S rDNA gene representing 'bacteria' increased transitorily, while the amount of 18S rDNA gene representing fungi decreased in soil. In addition, comparison of atzC QC-PCR results wit…

[SDE] Environmental SciencesDNA BacterialTime Factors[SDV]Life Sciences [q-bio]Microbial metabolismcomplex mixturesPolymerase Chain ReactionMicrobiology03 medical and health scienceschemistry.chemical_compoundRNA Ribosomal 16SRNA Ribosomal 18SAtrazineFood scienceBiomassDNA FungalSoil MicrobiologyComputingMilieux_MISCELLANEOUS0303 health sciencesbiologyBacteria030306 microbiologyHerbicidesFungi04 agricultural and veterinary sciencesGeneral MedicineBiodegradationPesticidebiology.organism_classificationSoil contamination[SDV] Life Sciences [q-bio]Microbial population biologychemistryInsect ScienceCalibration[SDE]Environmental Sciences040103 agronomy & agriculture0401 agriculture forestry and fisheriesAtrazineAgronomy and Crop ScienceSoil microbiologyBacteria
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Déterminisme du pouvoir protecteur de Fusarium oxysporum : recherche de gènes impliqués dans l'interaction protectrice avec la tomate

2007

Fusarium oxysporum is a common soil borne fungus, well represented in every type of soils, throughout the world. This species includes pathogenic strains inducing severe diseases in many crops and strains able to protect a plant against the infection by a pathogenic strain. The protective strains are not only non pathogenic strains isolated from suppressive soils but also pathogenic strains applied to a non host plant. The protective capacity of these strains is mainly based on mechanisms of competition and induced resistance of the plant The main objective of this work was to identify fungal genes involved in the protective capacity of these strains and associated to the elicitation of pla…

[SDE] Environmental SciencesFom24gène d’origine végétale et fongiquerapid subtraction hybridizationhybridation soustractive rapideactivité protectricebiocontrol capacitydifferentially expressed geneFusarium oxysporum[SDV] Life Sciences [q-bio]plant geneexpression différentiellefungal genemutant rev157
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Toward the Identification of Two Glycoproteins Involved in the Stomatal Deregulation of Downy Mildew–Infected Grapevine Leaves

2015

SPE Pôle IPM UB; International audience; Stomata remain abnormally opened and unresponsive to abscisic acid in grapevine leaves infected by downy mildew. This deregulation occurs from 3 days post inoculation and increases concomitantly with leaf colonization by the pathogen. Using epidermal peels, we demonstrated that the active compound involved in this deregulation is located in the apoplast. Biochemical assays showed that the active compound present in the apoplastic fluids isolated from Plasmopara viticola infected grapevine leaves (IAF) is a CysCys bridge-independent, thermostable and glycosylated protein. Fractionation guided assays based on chromatography / stomatal response and prot…

[SDE] Environmental SciencesProteomicsPhysiology[SDV]Life Sciences [q-bio]stomataMolecular Sequence DataPlant EpidermisFungal ProteinsCell wallPlasmoparaPlasmopara viticolachemistry.chemical_compoundCell WallBotany[SDV.BV]Life Sciences [q-bio]/Vegetal Biology[SDV.BV] Life Sciences [q-bio]/Vegetal BiologyComputer SimulationVitisAmino Acid SequencePathogenAbscisic acidPhylogenyproteomicGlycoproteinsPlant DiseasesPlant Proteinsplant-microbe interactionFungal proteinSequence Homology Amino AcidbiologyfungiPlant Stomatafood and beveragesGeneral MedicineChromatography Ion Exchangebiology.organism_classificationApoplast[SDV] Life Sciences [q-bio]Plant LeavesOomycetesBiochemistrychemistryVitis viniferaHost-Pathogen InteractionsPlant Stomata[SDE]Environmental SciencesDowny mildewguard cellAgronomy and Crop ScienceMolecular Plant-Microbe Interactions®
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