Search results for "SER"

showing 10 items of 22769 documents

Formation of dibutyl carbonate and butylcarbamate via CO2 insertion in titanium(IV) butoxide and reaction with n-butylamine

2016

Abstract The species resulting from insertion of 12CO2 and 13CO2 into titanium(IV) butoxide is for the first time fully characterized by means of infrared and nuclear magnetic resonance spectroscopy. Results show formation of Ti-monobutylcarbonate, that easily undergoes nucleophilic attack by an aliphatic amine. The hydrolysis of the resulting species produces butylcarbamate and dibutylcarbonate as the only main products. Characterization results of the carbonate-like adduct, along with its reactivity with amine molecules open the route to new ways of CO2 utilization as building block for valuable organic compounds.

010405 organic chemistryChemistryProcess Chemistry and Technologyn-Butylaminechemistry.chemical_elementNuclear magnetic resonance spectroscopy010402 general chemistry01 natural sciences0104 chemical sciencesAdductHydrolysischemistry.chemical_compoundNucleophilePolymer chemistryChemical Engineering (miscellaneous)Organic chemistryReactivity (chemistry)Amine gas treatingSettore CHIM/07 - Fondamenti Chimici Delle TecnologieWaste Management and DisposalTitaniumDibutyl carbonate CO2 insertion Titanium alkoxides Carbamate
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Bowl-shape electron donors with absorptions in the visible range of the solar spectrum and their supramolecular assemblies with C 60

2012

We describe the synthesis, electronic, optical and photophysical properties of a family of three electron-donor bowl-shaped organic molecules that absorb light in the whole range of the visible spectrum (up to 800 nm in one case), and associate C60 in solution with binding constants in the range of 104–102 M−1 as measured from both UV-vis and fluorescence titrations in several solvents. These molecules are π-extended derivatives of tetrathiafulvalene, based on a truxene core to which two or three units of dithiole are covalently attached. The inclusion of the bulky dithiole groups is responsible for their bowl-shape geometry, which allows them to associate with C60, and their electron-donor…

010405 organic chemistrySupramolecular chemistryGeneral Chemistry010402 general chemistryPhotochemistry01 natural sciences0104 chemical sciencesPhotoexcitationchemistry.chemical_compoundchemistryIntramolecular forceUltrafast laser spectroscopyDensity functional theoryAbsorption (chemistry)TetrathiafulvaleneVisible spectrum
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Dietary and Household Sources of Prenatal Exposure to Polybrominated Diphenyl Ethers (PBDEs) in the INMA Birth Cohort (Spain)

2016

This study looked at predictors of exposure to polybrominated diphenyl ethers (PBDEs) with a focus on dietary and household-level factors. Concentrations of BDE-47, -99, -153, and -209 and their sum (∑PBDEs) were measured in cord serum. Spanish women (n = 541) completed two semiquantitative food frequency questionnaires during the first and third trimesters of pregnancy. The daily mean intake (grams) of eggs, dairy products, meat, cereals and pasta, vegetables and pulses, fruits, shellfish and cephalopods, and fish, and the weekly mean intake (servings) of lean, large oily, other oily, and other fish from both questionnaires were averaged. Information on house size, curtains and carpets at …

010501 environmental sciencesThird trimester01 natural sciences03 medical and health sciences0302 clinical medicinePolybrominated diphenyl ethersPregnancyCORD SERUMEnvironmental healthHalogenated Diphenyl EthersAnimalsHumansEnvironmental ChemistryMedicine030212 general & internal medicinePrenatal exposure0105 earth and related environmental sciencesPregnancyFood frequencybusiness.industryGeneral Chemistrymedicine.diseaseDiet3. Good healthSeafoodSpainPrenatal Exposure Delayed EffectsEnvironmental chemistryGestationFemalebusinessBirth cohortEnvironmental Science & Technology
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Dimensionless Stage-Discharge Relationship for a Non-Linear Water Reservoir: Theory and Experiments

2020

In the field of hydrology, stage&ndash

010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technologyOceanography01 natural sciencesWater balanceWater reservoirSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-Forestali020701 environmental engineeringlcsh:ScienceWaste Management and Disposal0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyMathematicsConservation of energyMechanicsDischarge coefficientstage-discharge relationshipanalytical solutionNonlinear systemexperimental testContinuity equationlcsh:Qnon-linear reservoirDimensionless quantity
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Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

2020

We present measurements of the large-scale cosmic-ray anisotropies in right ascension, using data collected by the surface detector array of the Pierre Auger Observatory over more than 14 years. We determine the equatorial dipole component, ~d⊥, through a Fourier analysis in right ascension that includes weights for each event so as to account for the main detector-induced systematic effects. For the energies at which the trigger efficiency of the array is small, the “East-West” method is employed. Besides using the data from the array with detectors separated by 1500 m, we also include data from the smaller but denser sub-array of detectors with 750 m separation, which allows us to extend …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsAstrophysicsanisotropy [cosmic radiation]Amplitude01 natural sciencessurface [detector]010303 astronomy & astrophysicsRight ascensionastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSGalactic CenterAstrophysics::Instrumentation and Methods for AstrophysicsCosmic RaysAugerobservatoryAmplitudePhysics::Space PhysicsAstrophysics - High Energy Astrophysical PhenomenaExtragalactic cosmic rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raycosmic radiation: anisotropyExtragalactic cosmic rayGalactic center0103 physical sciencesHigh Energy PhysicsPierre auger observatory0105 earth and related environmental sciencesPierre Auger Observatorydetector: surfaceFísicaAstronomy and AstrophysicsCosmic rayefficiency [trigger]GalaxyDipole* Automatic Keywords *Space and Planetary ScienceExperimental High Energy Physicstrigger: efficiencyddc:520galaxyDipoleObservatoryEnergy (signal processing)anisotropiesRight ascension[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)dipoleThe Astrophysical Journal
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A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

2020

Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and other detectors of electromagnetic radiation in several bands. The Pierre Auger Observatory is sensitive to neutrinos in the energy range from 100 PeV to 100 EeV and in the zenith-angle range from θ = 60° to θ = 95°, where the zenith angle is measured from the vertical direction. No neutrinos from the direction of TXS 0506+056 have been found. The results were analyzed in three periods: One of 6 m…

010504 meteorology & atmospheric sciencesAstronomyAstrophysicspower spectrum7. Clean energy01 natural sciencesIceCubeObservatoryMAGIC (telescope)UHE Cosmic Rays010303 astronomy & astrophysicsHigh energy astrophysics Neutrino astrony Blazars Transient sources Active galaxiesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for Astrophysicsneutrino: UHEUHE [neutrino]AugerobservatoryHigh energy astrophysics; Neutrino astronomy; Blazars; Transient sources; Active galaxiesNeutrino detectorNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsradiation: electromagneticHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGLASTblazar0103 physical sciencesNeutrinoHigh Energy PhysicsZenithAstrophysique0105 earth and related environmental sciencesPierre Auger ObservatoryFísicaAstronomy and AstrophysicsAstronomiesensitivityMAGICTransient sourcesSciences de l'espaceelectromagnetic [radiation]13. Climate actionSpace and Planetary Sciencegamma rayExperimental High Energy PhysicsActive galaxiesddc:520spectralNeutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Blazars
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A 3-Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic-Ray Observatory

2020

The time and location of the 1,598 verified and reconstructed elves, used for the analysis showcased in this paper, are publicly available on the website of the Pierre Auger Observatory (https://www.auger.org/ index.php/science/data). We wish to thank the World Wide Lightning Location Network (http://wwlln.net), a collaboration among over 50 universities and institutions, for providing the lightning location data used in this paper. We acknowledge Robert Marshall for providing one of the most advanced elve simulations to the public, a key tool in understanding the elves observed by the Pierre Auger Observatory. The successful installation, commissioning, and operation of the Pierre Auger Ob…

010504 meteorology & atmospheric sciencesAstronomyField of view010502 geochemistry & geophysics01 natural sciences7. Clean energyAugerlcsh:QB1-991ObservatoryultravioletStormddc:550UHE Cosmic Raystime resolutionCosmic-ray observatoryPhysicslcsh:QE1-996.5astro-ph.GeologyAugerwidth [beam]IonosphereField of viewGeologylcsh:AstronomyUHE [cosmic radiation]Environmental Science (miscellaneous)horizonLightningddc:530High Energy PhysicsIonosphereCosmic-ray observatory0105 earth and related environmental sciencesfluorescence [detector]backgroundFísicaAstronomyStormsensitivityLightningopticslcsh:GeologyElves UV fluorescence detectorsThunderstorm13. Climate actionExperimental High Energy PhysicsnetworkThunderstormGeneral Earth and Planetary SciencesElvesObservatory
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Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2015–2018

2020

AbstractThis paper is devoted to the discovery of 37 asteroids at the Baldone Astrophysical Observatory (MPC 069) from 2015 to 2018, and one of dynamically interesting Mars-crosser (MC) observed at the Baldone Astrophysical Observatory, namely 2008 LX16. In Baldone Observatory, was independently discovered the Near-Earth Object 2018 GE3 on the image of 13 April 2018. Also, the NEO 2006 VB14 was observed doing its astrometry and photometry. Moreover, we observed asteroids 1986 DA and 2014 LJ1. We computed orbits and analyzed the orbital evolution of these asteroids. 566 positions and photometric observations of NEO objects 345705 (2006 VB14) and 6178 (1986 DA) were obtained with Baldone Schm…

010504 meteorology & atmospheric sciencesAstronomyorbitsAstronomyQB1-991Astronomy and AstrophysicsAstrometryEphemeris01 natural sciencesAstrobiologySpace and Planetary ScienceAsteroidObservatory0103 physical sciencesminor planetsastrometryminor planets ; asteroids ; astrometryObservational studyasteroids: search010303 astronomy & astrophysicsGeology0105 earth and related environmental sciencesOpen Astronomy
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Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020

We study the impact of gas accretion on the orbital evolution of black-hole binaries initially at large separation in the band of the planned Laser Interferometer Space Antenna (LISA). We focus on two sources: (i)~stellar-origin black-hole binaries~(SOBHBs) that can migrate from the LISA band to the band of ground-based gravitational-wave observatories within weeks/months; and (ii) intermediate-mass black-hole binaries~(IMBHBs) in the LISA band only. Because of the large number of observable gravitational-wave cycles, the phase evolution of these systems needs to be modeled to great accuracy to avoid biasing the estimation of the source parameters. Accretion affects the gravitational-wave p…

010504 meteorology & atmospheric sciencesAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)Observableastro-ph.HE; astro-ph.HE; General Relativity and Quantum Cosmologygas: accretionblack holes gravitational wavesobservatoryInterferometrygravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenainterferometermedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionelectromagnetic field: productionGeneral Relativity and Quantum Cosmologybinary: coalescencestatistical analysisSettore FIS/05 - Astronomia e Astrofisicagravitation: weak field0103 physical sciencesnumerical calculationsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLISAGravitational wavegravitational radiationOrder (ring theory)black hole: accretionAstronomy and Astrophysicsblack holesgravitational radiation detectorRedshiftBlack holeblack hole: binarySpace and Planetary ScienceSkygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray: detectorThe Astrophysical Journal
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IceCube search for neutrinos coincident with compact binary mergers from LIGO-Virgo's first gravitational-wave transient catalog

2020

Using the IceCube Neutrino Observatory, we search for high-energy neutrino emission coincident with compact binary mergers observed by the LIGO and Virgo gravitational-wave (GW) detectors during their first and second observing runs. We present results from two searches targeting emission coincident with the sky localization of each GW event within a 1000 s time window centered around the reported merger time. One search uses a model-independent unbinned maximum-likelihood analysis, which uses neutrino data from IceCube to search for pointlike neutrino sources consistent with the sky localization of GW events. The other uses the Low-Latency Algorithm for Multi-messenger Astrophysics, which …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsBayesian7. Clean energy01 natural sciencesNeutrino astronomy; High energy astrophysics; Gravitational waveslocalizationIceCubeIceCube Neutrino ObservatoryGravitational wavesparticle source [neutrino]0103 physical sciencesLIGO010303 astronomy & astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGravitational wavegravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsLIGOobservatorymessengerMassless particleVIRGONeutrino detector13. Climate actionSpace and Planetary ScienceNeutrino astronomycompact [binary]Physique des particules élémentairesddc:520High Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsLepton
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