Search results for " method"

showing 10 items of 10455 documents

Orobanche rameuse du tabac (Phelipanche ramosa L.) : Identifier de nouvelles solutions conventionnelles et de biocontrôle

2019

The branching broomrape, Phelipanche ramosa L. is an obligate parasitic plant, which in a few years became a major agronomic problem for tobacco crops in France. Two approaches, aiming at controlling broomrape were tested within the framework of the ELIOT project grouping Arvalis, the CT2F cooperative and the INRA center of Dijon. The first relates to sulfonylurea herbicides, including rimsulfuron and sulfosulfuron and a systemic herbicide of the cyclohexanediones family, clethodim. The results, although instructive, do not reflect an effective control of broomrape. The second approach deals with the search for soil-borne fungi that are pathogenic to broomrape. A large number of fungal stra…

[SDE] Environmental Sciencesmycoherbicidechemical method[SDV]Life Sciences [q-bio]tabacco croptabac[SDV] Life Sciences [q-bio]rimsulfuron[SDE]Environmental Scienceslutte herbicidemycoherbicide.Phelipanche ramosa L.;tabac;rimsulfuron;sulfosulfuron;lutte herbicide;mycoherbicide;crop;rimsulfuron;sulfosulfuron;chemical method;mycoherbicidessulfosulfuron[SDV.BV]Life Sciences [q-bio]/Vegetal BiologyPhelipanche ramosa L.crop[SDV.BV] Life Sciences [q-bio]/Vegetal Biology
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Prevalence of Mycobacterium bovis in agroecosystems : analysis of potential environmental reservoirs (soil, fresh water, soil fauna and aquatic fauna…

2016

Bovine tuberculosis is an infectious disease caused by Mycobacterium bovis. This disease affects cattle, and many species of domestic and wild mammals, and humans. The circulation of the bacteria in various multi-host systems promotes the maintenance of the disease and the contamination of cattle in the vicinity. Beside direct transmission of the bacteria through the respiratory route, indirect transmission, through inhalation or ingestion of environmental matrices contaminated by an infected animal excretory, is suspected in several countries. Environmental contamination with M. bovis appears to be a crucial factor in the persistence of the infection in multi-host systems. In Côte d'Or, a …

[SDE] Environmental Sciencessol[SDV]Life Sciences [q-bio]EnvironmentWildlife[ SDV.MP.BAC ] Life Sciences [q-bio]/Microbiology and Parasitology/Bacteriology[SDV.BBM.BM] Life Sciences [q-bio]/Biochemistry Molecular Biology/Molecular biology[ SDV.BA ] Life Sciences [q-bio]/Animal biologyWild animalsfècesSoilFeces[SDV.EE.ECO]Life Sciences [q-bio]/Ecology environment/Ecosystemseauculture based method[SDV.EE.ECO] Life Sciences [q-bio]/Ecology environment/Ecosystemsfeces analysis[SDV.BV] Life Sciences [q-bio]/Vegetal BiologyComputingMilieux_MISCELLANEOUS[SDE.IE]Environmental Sciences/Environmental Engineering[SDV.BA]Life Sciences [q-bio]/Animal biologyWater[SDV.BBM.BM]Life Sciences [q-bio]/Biochemistry Molecular Biology/Molecular biology[SDV.EE.IEO] Life Sciences [q-bio]/Ecology environment/Symbiosisbovins[SDV.MP.BAC]Life Sciences [q-bio]/Microbiology and Parasitology/BacteriologyMycobacterium bovisenvironnementsoil ecologyfaune sauvageculture[SDV] Life Sciences [q-bio]qPCRCattle[SDE.IE] Environmental Sciences/Environmental Engineering[SDV.MP.BAC] Life Sciences [q-bio]/Microbiology and Parasitology/Bacteriology[SDV.EE.IEO]Life Sciences [q-bio]/Ecology environment/Symbiosis
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

2008

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the ighest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than ~6 x 1019 eV and AGN at a distance less than ~75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate fro…

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyOsservatorio Pierre AugerAstrophysicsGALAXY CLUSTER SURVEYAstrophysicsauger01 natural sciencesHigh energy cosmic rayRaggi cosmiciAstrophysical jetGMFObservatoryUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsBL-LACERTAEGreisen–Zatsepin–Kuz’min effect[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGINUHECRAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKRadiación cósmicaAnisotropíaCATALOGobservatoryddc:540EGMFCUTOFFComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRELATIVISTIC JETSActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaCosmic background radiationFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATION[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesextra-galacticPARTICLESAGNAstrophysics::Galaxy AstrophysicsCiencias ExactasPierre Auger ObservatoryANISOTROPYhigh energy cosmic raysSciami atmosferici010308 nuclear & particles physicsFísicaAstronomyAstronomy and AstrophysicsCENTAURUSGalaxyExperimental High Energy Physics
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Observation of the suppression of the flux of cosmic rays above 4x10^19eV

2008

The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E-γ, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), steepening to 4.2 ± 0.4(stat) ± 0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical Phenomenaenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxOsservatorio Pierre Augerspectral indexCosmic rayparticle fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEXTENSIVE AIR-SHOWERSAstrophysicsUPPER LIMIT01 natural sciencesPower lawAugerNuclear physicsENERGY[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmicicosmic rays0103 physical sciencesddc:550Particle flux010303 astronomy & astrophysicsCiencias ExactasPhysicsPierre Auger ObservatorySpectral indexSPECTRUM[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaARRAYHigh Energy Physics::ExperimentSciami atmosferici estesiEnergy (signal processing)
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Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector

2010

The ANTARES high energy neutrino telescope is a three-dimensional array of about 900 photomultipliers distributed over 12 mooring lines installed in the Mediterranean Sea. Between February and November 2007 it acquired data in a 5-line configuration. The zenith angular distribution of the atmospheric muon flux and the associated depth-intensity relation are measured and compared with previous measurements and Monte Carlo expectations. An evaluation of the systematic effects due to uncertainties on environmental and detector parameters is presented.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsMonte Carlo methodAtmospheric muonsFluxNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)WATER010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAY CASCADES NEUTRINO TELESCOPE PERFORMANCE GENERATOR SYSTEM MODULE LIGHT WATER SITESITEMUON FLUXLIGHTddc:540Física nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsMODULEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayParticle detectorCOSMIC-RAY CASCADESNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]depth-intensity relation0103 physical sciencesatmospheric muons; depth-intensity relation; neutrino telescope14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithRemote sensingatmospheric muonsDepth-intensity relation010308 nuclear & particles physicsneutrino telescopeAstronomy and AstrophysicsCOSMIC RAYSPERFORMANCEGENERATORMeasuring instrumentHigh Energy Physics::ExperimentUNDERWATER DETECTORSYSTEM
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory

2012

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 1018 eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 1018 eV from stationary Galactic …

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Radiación CósmicaAstronomyMilky WayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesGALACTIC MAGNETIC-FIELDSAuger[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]cosmic raysObservatory0103 physical sciencesastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Ciencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsPierre Auger ObservatoryANISOTROPY010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFísicaAstronomy and AstrophysicsENERGY-SPECTRUMUltra-High Energy Cosmic Rays Pierre Auger Observatory Large Scale AnisotropiesSpace and Planetary Scienceastroparticle physicsExperimental High Energy PhysicsROTATIONARRAYFísica nuclearAstroparticle physicsRight ascensionAstrophysics - High Energy Astrophysical Phenomena
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VizieR Online Data Catalog: 46 open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018)

2018

We have determined the membership of 46 open clusters. For the nine clusters within 250pc we determined optimised parallaxes based on the combined information extracted from the measured parallax and proper motion values. These clusters are : in Tables A1a & A3: alphaPer, Blanco1, ComaBer, Hyades, IC2391, IC2602, NGC2451A, Pleiades, Praesepe. The remaining 37 clusters are in Table A1b & A4: Coll140, IC4651, IC4665, IC4725, IC4756, NGC0188, NGC0752, NGC0869, NGC0884, NGC1039, NGC1901, NGC2158, NGC2168, NGC2232, NGC2323, NGC2360, NGC2422, NGC2423, NGC2437, NGC2447, NGC2516, NGC2547, NGC2548, NGC2682, NGC3228, NGC3532, NGC6025, NGC6281, NGC6405, NGC6475, NGC6633, NGC6774, NGC6793, NGC7092, Sto…

[SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Parallaxes: trigonometricClusters: openProper motions
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Ariel: Enabling planetary science across light-years

2021

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. During its 4-year mission, Ariel will study what exoplanets are made of, how they formed and how they evolve, by surveying a diverse sample of about 1000 extrasolar planets, simultaneously in visible and infrared wavelengths. It is the first mission dedicated to measuring the chemical composition and thermal structures of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of the Solar System. The payload consists of an off-axis Cassegrain telescope (primary mirror 1100 mm x 730 mm e…

[SDU] Sciences of the Universe [physics]Earth and Planetary Astrophysics (astro-ph.EP)[SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Settore FIS/05 - Astronomia E Astrofisica[SDU]Sciences of the Universe [physics][SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]FOS: Physical sciencesAstrophysics - Instrumentation and Methods for AstrophysicAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics - Earth and Planetary Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
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Question on ipm: A case study on lemon juice

2012

International audience; In food product development, using consumers to obtain ideal products is becoming more frequent inrecent years. Despite being an economical way of optimizing products, relying on consumers is,however, not yet widely accepted in the sensory community. The main objectives of this study were toevaluate (1) whether the stability of ideal intensities and ideal products could be improved byproviding a frame of references when consumers perform the Ideal Profile Method (IPM) and (2) theeffect of the order of the questions on consumers‘ responses.In the present study, sixty participants conducted two tasks: (1) rating the perceived and idealintensities of attributes and (2) …

[SDV.AEN] Life Sciences [q-bio]/Food and NutritionFood product developmentIdeal Profile MethodOrder effect[SDV.AEN]Life Sciences [q-bio]/Food and Nutrition
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Sensory science: new needs and challenges

2018

[SDV.AEN] Life Sciences [q-bio]/Food and Nutritionbiasfat reductionsensory methodssugar reductionsalt reduction[SDV.AEN]Life Sciences [q-bio]/Food and Nutrition
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