0000000001145269

AUTHOR

B. Garcia

showing 14 related works from this author

Satisfaction of patients fitted with implant-retained overdentures

2011

Objective: to evaluate patient satisfaction with implant-retained overdentures, and its relationship with age, sex, period of follow-up, the rehabilitated jaw (maxilla, mandible or both), number of implants, splinting, type of attachment and the antagonist.Material and methods: the study comprised patients with overdentures fitted between January 1996 and June 2007, and with a minimum follow-up of one year. Data regarding patients and prostheses were collected. The patients indicated their overall satisfaction on a visual analogue scale (VAS) from 0 to 10, as well as satisfaction for individual items such as aesthetics, speech, mastication, prosthetic stability and selfesteem. These data we…

business.industryVisual analogue scalemedicine.medical_treatmentMandibleDentistry:CIENCIAS MÉDICAS [UNESCO]ProsthesisPatient satisfactionOtorhinolaryngologyStatistical significanceMaxillaUNESCO::CIENCIAS MÉDICASMedicineSurgeryImplantbusinessGeneral DentistryMasticationMedicina Oral Patología Oral y Cirugia Bucal
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Two guaianolides from Centaurea collina

1987

Abstract Two guaianolides isolated from the aerial parts of Centaurea collina were identified as 3β-hydroxy-8α-epoxymethylacriloiloxy-4(15),10(14),11(13 and its 11β,13-dihydro derivative by spectroscopic methods.

chemistry.chemical_compoundChemistryBotanyPlant ScienceGeneral MedicineHorticultureMolecular BiologyBiochemistryCentaurea collinaDerivative (chemistry)Phytochemistry
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A Bioinspired Approach to Tri-nor-guaianes. Synthesis of (−)-Clavukerin A

2006

A bioinspired approach to tri-nor-guaianes by degradation of the C-7 side chain of related guaia-11-enes is described. In this approach (-)-clavukerin A (1) is obtained by selective ozonolysis-Criegge rearrangement of (+)-1alphaH,7alphaH,10alphaH-guaia-4,11-dien-3-one (4) to afford 7beta-hydroxy and 7beta-acetoxy tri-nor-guaiane derivatives 6 and 7, respectively, which after elimination and deoxygenation give the title compound. The starting guaiadienone is readily obtained from commercially available santonin or (+)-dihydrocarvone.

PharmacologyOzonolysisMolecular StructureOrganic ChemistryPharmaceutical ScienceStereoisomerismSesquiterpeneChemical synthesisAnalytical ChemistrySesquiterpenes Guaianechemistry.chemical_compoundComplementary and alternative medicinechemistryDrug DiscoverySide chainMolecular MedicineOrganic chemistryCycloheptanesPolycyclic Aromatic HydrocarbonsEnantiomerSelectivityDeoxygenationJournal of Natural Products
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Ultrasound assisted reductive cleavage of sesquiterpene γ-enonelactones

1995

Abstract Ultrasound enhances the rate of reductive cleavage of the C 6 -oxygen bond of several cis - and trans - sesquiterpene γ-enonelactones. Interestingly ultrasound overrides the stereoelectronic requirements for the reductive cleavage of the most usually occurring sesquiterpene trans -lactones.

chemistry.chemical_compoundchemistryStereochemistryReductive cleavageOrganic ChemistryDrug DiscoveryOrganic chemistrychemistry.chemical_elementSesquiterpeneUltrasound assistedBiochemistryOxygenTetrahedron Letters
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ChemInform Abstract: The Synthesis of Bioactive Sesquiterpenes from Santonin

2010

Abstract This article reviews the literature published in the last decade dealing with the transformation of α-santonin into bioactive or potentially bioactive sesquiterpenes. A number of syntheses starting from 8α-hydroxysantonin (artemisin) have also been included. Special emphasis has been placed on synthesized products that show biological activity. Major advances in this field include the application of new reagents and methodologies for the structural modification of the santonin skeleton and functionality, and its transformation into other sesquiterpenes, especially sesquiterpene lactones. The review has been organised into five parts: 1. Introduction: An overview of the structure an…

Terpenechemistry.chemical_classificationchemistry.chemical_compoundChemistryOrganic chemistryMoietyGeneral MedicineSesquiterpeneLactoneSantoninChemInform
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Flavonoids, flavonolignans and a phenylpropanoid from Onopordon corymbosum

1990

Abstract The aerial parts of Onopordon corymbosum afforded seven flavonoids, 3-(3,4-dihydroxyphenyl)-1-propanol and two flavonolignans, hydnocarpin and the new 5′'-methoxy-hydnocarpin.

Flavonolignanschemistry.chemical_classificationPhenylpropanoidChemistryHydnocarpinBotanyFlavonoidPlant ScienceGeneral MedicineHorticultureMolecular BiologyBiochemistryPhytochemistry
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A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

2010

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierr…

Angstrom exponentAstronomyAstrophysics01 natural sciencesAugerCROSS-SECTIONSCOSMIC-RAY SHOWERSObservatoryDEPENDENCEHigh-Energy Cosmic Ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Lidar[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ANGSTROM EXPONENTPierre Auger ObservatoryBi-static lidarELECTRONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMULTIPLE-SCATTERINGLight emissionFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLIGHT-EMISSIONAstrophysics - Cosmology and Nongalactic Astrophysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Extensive air showerFOS: Physical sciencesCosmic raySURFACE DETECTORAir fluorescence method0103 physical sciencesExtensive air showersRECONSTRUCTIONAerosolInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryAerosolsCalorimeter (particle physics)Atmospheric effect010308 nuclear & particles physicsAtmosphereFísicaAstronomy and AstrophysicsCosmic rays; Extensive air showers; Air fluorescence method; Atmosphere; Aerosols; Lidar; Bi-static lidarCosmic rayNITROGENAir showerFluorescence Telescopes13. Climate actionExperimental High Energy PhysicsAEROSSOL
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Syntheses of (+)-alismoxide and (+)-4-epi-alismoxide.

2006

The first total syntheses of (+)-alismoxide and (+)-4-epi-alismoxide are reported. Formal chemo-, regio-, and stereoselective addition of water to 10alpha-acetoxy-1alphaH,5betaH-guaia-3,6-diene afforded the target compounds after reduction. The absolute stereochemistry of (+)-alismoxide has been established. The low [alpha](D) +8.6 value indicates that significant amounts of alismoxide result from biosynthetic processes. Furthermore, the structure of the natural guaienediol isolated from Silphium perfoliatum has been corrected to (-)-alismoxide.

GuaninebiologyMolecular StructureChemistryStereochemistryOrganic ChemistryAbsolute configurationTotal synthesisRegioselectivityWaterStereoisomerismStereoisomerismAsteraceaebiology.organism_classificationChemical synthesisAzulenesSesquiterpenes GuaianeSilphium perfoliatumStereoselectivityChemoselectivityThe Journal of organic chemistry
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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

2007

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar…

Active galactic nucleus[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]Cosmic background radiationFOS: Physical sciencesFluxOsservatorio Pierre AugerCosmic rayanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmici0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsBackground radiationNuclei galattivi attiviPhysicsPierre Auger ObservatorySPECTRUMMultidisciplinary[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMedicine (all); MultidisciplinaryMedicine (all)Settore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)angular dependence [cosmic radiation]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaExperimental High Energy Physicsddc:500Energy (signal processing)experimental results
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The Synthesis of Bioactive Sesquiterpenes from Santonin

2000

Abstract This article reviews the literature published in the last decade dealing with the transformation of α-santonin into bioactive or potentially bioactive sesquiterpenes. A number of syntheses starting from 8α-hydroxysantonin (artemisin) have also been included. Special emphasis has been placed on synthesized products that show biological activity. Major advances in this field include the application of new reagents and methodologies for the structural modification of the santonin skeleton and functionality, and its transformation into other sesquiterpenes, especially sesquiterpene lactones. The review has been organised into five parts: 1. Introduction: An overview of the structure an…

chemistry.chemical_classificationchemistry.chemical_compoundChemistryStereochemistryMoietyOrganic chemistrySesquiterpeneLactoneSantonin
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ChemInform Abstract: Ultrasound-Assisted Reductive Cleavage of Sesquiterpene γ- Enonelactones.

2010

Abstract Ultrasound enhances the rate of reductive cleavage of the C 6 -oxygen bond of several cis - and trans - sesquiterpene γ-enonelactones. Interestingly ultrasound overrides the stereoelectronic requirements for the reductive cleavage of the most usually occurring sesquiterpene trans -lactones.

Terpenechemistry.chemical_compoundchemistryStereochemistryReductive cleavagechemistry.chemical_elementGeneral MedicineSesquiterpeneUltrasound assistedOxygenChemInform
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Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

2016

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Hadronic interaction[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsCOLLISIONSAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesGeneral Physics and AstronomyCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciencesCalibrationHigh Energy PhysicsUHE Cosmic Rays010306 general physicsParticle PhysicsCosmic raysGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryEnergyMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaInteraction modelASTROFÍSICAHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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Direct measurement of the muonic content of extensive air showers between 2× 1017 and 2×1018 eV at the Pierre Auger Observatory

2020

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10 17 and 2 × 10 18 eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector …

Muon detector ultra-high energy cosmic raysmuonsUHE Cosmic Rays
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Upper limit on the cosmic-ray photon flux above 1019 eV using the surface detector of the Pierre Auger Observatory

2008

A method is developed to search for air showers initiated by photons using data recorded by the surface detector of the Auger Observatory. The approach is based on observables sensitive to the longitudinal shower development, the signal risetime and the curvature of the shower front. Applying this method to the data, upper limits on the flux of photons of 3.8 x 10-3, 2.5 x 10-3; and 2.2 x 10-3 km-2 sr-1 yr-1 above 1019 eV, 2 x 1019 eV; and 4 x 1019 eV are derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%, and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic models of sources of cosmic rays. The results also show that the approach adopted…

Photon[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyFluxFOS: Physical sciencesOsservatorio Pierre AugerCosmic rayFotonesAstrophysicsAstrophysics7. Clean energy01 natural sciencesAugerNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)Raggi cosmiciultra high energy photonsCascada atmosféricaObservatory0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatoryPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaAstronomy and AstrophysicsPierre Auger ObservatoryEnergia ultra altaCosmic rayHigh Energy Physics - PhenomenologyPair production13. Climate actionFotoniExperimental High Energy Physicsddc:540flux upper limitNeutrinoSciami atmosferici estesi
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