Search results for "PTH"

showing 10 items of 458 documents

Terminal ligature of inferior thyroid arterhy branches during total thyroidectomy for multinodular goiter is associated with higher postoperative cal…

2010

Purpose: To evaluate the impact of truncal versus terminal branch ligature of the inferior thyroid artery (ITA) on postoperative calcium and PTH plasma levels in patients undergoing total thyroidectomy for multinodular goiter. Methods: A prospective randomized study was performed comparing a group of patients that underwent either truncal ligature of the ITA (group 1) or terminal ligature of ITA branches (group 2). Results: A series of 126 consecutive patients with non-toxic euthyroid multinodular goiter underwent total thyroidectomy. Truncal ligature of the ITA was performed in 63 patients (group 1) and terminal branch ITA ligature in 63 patients (group 2). Postoperative ionized serum calc…

AdultMaleendocrine systemmedicine.medical_specialtyendocrine system diseasesmedicine.medical_treatmentThyroid Glandchemistry.chemical_elementCalciumInferior thyroid arterhythyroidectomyPTHmedicine.arteryMultinodular goitermedicineHumansPostoperative PeriodProspective StudiesInferior thyroid arteryLigatureLigationTotal thyroidectomyGoiterbusiness.industryThyroidThyroidectomyArteriesGeneral Medicinemedicine.diseaseSurgerySettore MED/18 - Chirurgia Generalemedicine.anatomical_structurechemistryHypoparathyroidismParathyroid HormoneThyroidectomyCalciumFemalebusiness
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Assessment of Kinect V2 for elbow range of motion estimation in people with haemophilia using an angle correction model

2018

Introduction The joint range of motion (ROM) is an important clinical parameter used to assess the loss of functionality resulting from joint bleedings in people with haemophilia. These episodes require a close follow-up and, to decrease patients' hospital dependence, telemedicine tools are needed. Therefore, this study is aimed to analyse the validity of the Microsoft Kinect V2 sensor with corrected angle measurement to be used in the monitoring of elbow ROM in people with haemophilia. Methods A convenience sample of 10 healthy controls (CG) and 10 patients with haemophilia with elbow arthropathy (HG) participated in this study. Full ROM of elbow joints was measured in the frontal view wit…

AdultMalemedicine.medical_specialtyWilcoxon signed-rank testElbow030204 cardiovascular system & hematologyHemophilia AHaemophiliarange of motion03 medical and health sciences0302 clinical medicinePhysical medicine and rehabilitationElbow JointHemarthrosisArthropathymedicineElbow jointsupper extremityHumansRange of Motion ArticularGenetics (clinical)Models Statisticalbusiness.industryLimits of agreementhaemophilic arthropathy3D depth sensorHematologyGeneral Medicinemedicine.diseasemedicine.anatomical_structureGoniometerFemaleRange of motionbusinessgoniometry030215 immunology
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Symmetric bilateral implantation of a distance-dominant diffractive bifocal intraocular lens

2007

To assess visual results after symmetrical bilateral implantation of a distance-dominant bifocal diffractive intraocular lens (IOL).Fernández-Vega Ophthalmological Institute, Oviedo, Spain.Fifty patients had bilateral implantation of a distance-dominant diffractive bifocal 447D IOL (Acri.Tec GmbH) in a prospective study. Monocular and binocular best corrected distance visual acuities and best distance-corrected near visual acuity, binocular best distance-corrected intermediate visual acuity, and distance contrast sensitivity under photopic (85 cd/m(2)) and mesopic (5 cd/m(2)) conditions were determined.At the 6-month postoperative visit, the mean binocular best corrected distance acuity and…

AdultMalemedicine.medical_specialtygenetic structuresMesopic visionmedia_common.quotation_subjectmedicine.medical_treatmentVisual AcuityIntraocular lensContrast SensitivityNear acuityLens Implantation IntraocularOphthalmologymedicineHumansContrast (vision)Prospective StudiesAgedmedia_commonAged 80 and overLenses IntraocularDepth PerceptionVision BinocularPhacoemulsificationMonocularbusiness.industryDistance PerceptionPhacoemulsificationMiddle Agedeye diseasesSensory SystemsOphthalmologyPostoperative visitOptometryFemaleSurgerybusinessPhotopic visionJournal of Cataract and Refractive Surgery
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(Table 1) Age determination of sediment core SO147_106KL

2005

Here we present a high-resolution marine sediment record from the El Niño region off the coast of Peru spanning the last 20,000 years. Sea surface temperature, photosynthetic pigments, and a lithic proxy for El Niño flood events on the continent are used as paleo-El Niño-Southern Oscillation proxy data. The onset of stronger El Niño activity in Peru started around 17,000 calibrated years before the present, which is later than modeling experiments show but contemporaneous with the Heinrich event 1. Maximum El Niño activity occurred during the early and late Holocene, especially during the second and third millennium B.P. The recurrence period of very strong El Niño events is 60-80 years. El…

Age datedPiston corer (BGR type)SonneAge maximum/oldAge minimum/youngLaboratory code/labelAge dated error to youngerAge dated error to olderAge 14C calibratedDEPTH sediment/rockSO147Age 14C AMSAge model
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Lensless object scanning holography for two-dimensional mirror-like and diffuse reflective objects

2013

Recently proposed lensless object scanning holography (LOSH) [Opt. Express 20, 9382 (2012)] is a fully lensless method capable of improving the image quality in digital Fourier holography applied to one-dimensional (1D) reflective objects and it involves a very simplified experimental setup. LOSH is based on the recording and digital postprocessing of a set of digital lensless Fourier transform holograms, which finally results in a synthetic image with improved resolution, field-of-view (FOV), signal-to-noise ratio (SNR), and depth of field. In this paper, LOSH is extended to the cases of two-dimensional (2D) mirror-like and 1D diffuse-based objects. For 2D mirror-like objects, the experime…

ApertureImage qualityComputer sciencebusiness.industryHolographyImage processingSuperresolutionAtomic and Molecular Physics and Opticslaw.inventionSpeckle patternOpticslawDigital image processingDepth of fieldElectrical and Electronic EngineeringbusinessEngineering (miscellaneous)Image resolutionDigital holographyFresnel diffractionApplied Optics
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Imaging Quality of Bifocal Piggyback Intraocular Lens versus ReSTOR and TECNIS Multifocal Lenses

2009

Purpose The imaging quality provided by a piggyback integrated by a monofocal intraocular lens (IOL) + a bifocal IOL of zero power and +3.75 diopters of addition is compared with the optics quality of a simple multifocal IOL of the same power and addition. Methods The imaging quality was evaluated by determining the modulation transfer function (MTF), using an artificial eye simulating in vivo conditions of the anterior chamber, including an artificial cornea and a wet cell containing physiologic solution where the IOL was positioned. The MTFs of the bifocal piggyback for near and distance vision were measured, with pupil diameters of 3 and 5 mm, and compared with the MTFs of an equivalent …

Artificial corneaOptics and Photonicsmedicine.medical_specialtybusiness.product_categoryMaterials sciencemedicine.medical_treatmentVisual AcuityIntraocular lensEyeRefraction OcularPupil03 medical and health sciences0302 clinical medicineOptical transfer functionOphthalmologymedicineHumansMultifocal lensesDioptreLenses IntraocularDepth PerceptionStrehl ratioGeneral MedicineModels TheoreticalOphthalmologyImaging quality030221 ophthalmology & optometryArtificial Organsbusiness030217 neurology & neurosurgeryEuropean Journal of Ophthalmology
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

2014

The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60° and different energies of the primary particle. From these distributions, we define Xμmax as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of Xμmax as a useful observable to infer the mass compositi…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyCiencias Físicasmuonshadronic interaction modelsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentAuger//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Air showersProduction depthSURFACE DETECTOR ARRAY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh-Energy Cosmic Rays[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Pierre Auger ObservatoryObservableInstrumentation and Detectors (physics.ins-det)COSMIC-RAYSlongitudinal developmentCore (optical fiber)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayNuclear physicscosmic rays[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesextensive air showers[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)ZenithCiencias ExactasPierre Auger ObservatoryMuon010308 nuclear & particles physics[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Física//purl.org/becyt/ford/1.3 [https]ASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaMODELExperimental High Energy PhysicsHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [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]muonic componentSYSTEM
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Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

2012

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargüe and averaged monthly models, the utility of the GDAS data is shown.

AstronomyAtmospheric modelAtmospheric monitoringAtmospheric sciencesCosmic Rays Shower01 natural scienceslaw.inventionData assimilationlawcosmic rays; extensive air showers; atmospheric monitoring; atmospheric modelsDEPENDENCEATMOSFERA (OBSERVAÇÃO)TEMPERATUREPhysics::Atmospheric and Oceanic PhysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]Cascada atmosférica extensaOPTICAL DEPTH[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryAtmospheric temperatureRadiación cósmicaAtmosphere of EarthComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRadiosondeFísica nuclearREFRACTIVE-INDEXAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]MeteorologyAtmospheric MonitoringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic Rays ShowersEXTENSIVE AIR-SHOWERSCosmic RayAtmósferaWeather stationAtmospheric models0103 physical sciencesExtensive air showers010306 general physicsCosmic raysDETECTORCiencias ExactasPierre Auger ObservatoryAtmospheric models010308 nuclear & particles physicsFísicaAstronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsEMISSION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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X-ray spectroscopy of the ADC source X1822-371 with Chandra and XMM-Newton

2012

The eclipsing low-mass X-ray binary X1822-371 is the prototype of the accretion disc corona (ADC) sources. We analyse two Chandra observations and one XMM-Newton observation to study the discrete features and their variation as a function of the orbital phase, deriving constraints on the temperature, density, and location of the plasma responsible for emission lines. The HETGS and XMM/Epic-pn observed X1822-371 for 140 and 50 ks, respectively. We extracted an averaged spectrum and five spectra from five selected orbital-phase intervals that are 0.04-0.25, 0.25-0.50, 0.50-0.75, 0.75-0.95, and, finally, 0.95-1.04; the orbital phase zero corresponds to the eclipse time. All spectra cover the e…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral lineidentification line: formation stars: individual: X1822-371 X-rays: binaries X-rays: general [line]Settore FIS/05 - Astronomia E Astrofisica0103 physical sciencesOptical depth (astrophysics)line: identification line: formation stars: individual: X1822-371 X-rays: binaries X-rays: generalEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsLine-of-sight010308 nuclear & particles physicsResonanceAstronomy and AstrophysicsRadiusCoronaSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Air traffic and contrail changes during COVID-19 over Europe: A model study

2021

The strong reduction of air traffic during the COVID-19 pandemic provides a test case for the relation between air traffic density, contrails, and their radiative forcing of climate change. Air traffic and contrail cirrus changes are quantified for a European domain for March to August 2020 and compared to the same period in 2019. Traffic data show a 72 % reduction in flight distance compared with 2019. This paper investigates the induced contrail changes in a model study. The contrail model results depend on various methodological details tested in parameter studies. In the reference case, the reduced traffic caused an even stronger reduction in contrail length, partly because the w…

AtmosphereLongwaveEnvironmental scienceCirrusForcing (mathematics)Radiative forcingAtmospheric sciencesShortwaveWater vaporOptical depth
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