Search results for "basel"

showing 10 items of 332 documents

Improved femoral neck BMD in older Finnish women between 2002 and 2010.

2013

Abstract Purpose The number of hip fractures among Finns over 50-years of age rose constantly between 1970 and 1997, but since then, there has been a nationwide decline in incidence of hip fractures. One possible explanation, although not the only one, for the declining fracture rates, could be improved bone mineral density (BMD). The aim of this study was to evaluate differences in femoral neck BMD between older Finnish women born about a decade apart. Methods We compared the baseline data of two population-based samples of home-dwelling 70–80-year-old women who were initially recruited in exercise intervention studies ( N  = 216 in Cohort1, and N  = 389 in Cohort 2). Femoral neck BMD was …

medicine.medical_specialtymedicine.medical_treatmentOsteoporosisPopulationGeneral Biochemistry Genetics and Molecular BiologyCohort StudiesBone DensitymedicineHumanseducationFinlandOsteoporosis PostmenopausalFemoral neckAgedBone mineralAged 80 and overeducation.field_of_studyAnalysis of Variancebusiness.industryFemur NeckHip FracturesIncidence (epidemiology)IncidenceAge FactorsObstetrics and Gynecologyta3141Baseline datamedicine.diseaseBody Heightmedicine.anatomical_structureCohortPhysical therapyFemaleHormone therapybusinessDemographyMaturitas
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Ecologists overestimate the importance of predictor variables in model averaging: a plea for cautious interpretations.

2014

Abstract: Information-theory procedures are powerful tools for multimodel inference and are now standard methods in ecology. When performing model averaging on a given set of models, the importance of a predictor variable is commonly estimated by summing the weights of models where the variable appears, the so-called sum of weights (SW). However, SWs have received little methodological attention and are frequently misinterpreted. We assessed the reliability of SW by performing model selection and averaging on simulated data sets including variables strongly and weakly correlated to the response variable and a variable unrelated to the response. Our aim was to investigate how useful SWs are …

model selectionInformation theorymultimodel inferenceBayesian information criterionStatisticsEconometricsRange (statistics)Akaike Information Criterion[ SDV.EE.IEO ] Life Sciences [q-bio]/Ecology environment/Symbiosisbaseline sum of weightsSet (psychology)BiologyEcology Evolution Behavior and SystematicsMathematicsinformation theory[STAT.AP]Statistics [stat]/Applications [stat.AP]Ecological ModelingModel selection[ STAT.AP ] Statistics [stat]/Applications [stat.AP]model averagingBayesian information criterionChemistryVariable (computer science)Sample size determinationvariable importanceAkaike information criterion[SDV.EE.IEO]Life Sciences [q-bio]/Ecology environment/Symbiosis
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Long-baseline neutrino oscillation physics potential of the DUNE experiment

2020

The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and a full simulation and parameterized analysis of the near detector. Detailed uncertainties due to the flux prediction, neutrino interaction model, and detector effects are included. DUNE will resolve the neutrino mass ordering to a precision of 5σσ, for all δCPδCP values, after 2 years of running with the nominal detector design and beam configuration. It has the potential to observe charge-parity violation in the neutrino sector to a precision of 3σσ (5σσ) after an exposure of 5 (10) years, for 50% o…

neutriino-oskillaatioPhysics::Instrumentation and DetectorsilmaisimetHigh Energy Physics::Phenomenologyneutriinotlong-baseline neutrino oscillation physicsHigh Energy Physics::Experimenthiukkasfysiikka
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TANAMI II. Additional sources

2018

TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of -30{deg} declination including high-resolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and {gamma}-ray studies. We have previously published first-epoch 8.4GHz VLBI images of the parsec-scale structure of the initial sample. In this paper, we present images of 39 additional sources. The full sample comprises most of the radio- and {gamma}-ray brightest AGN in the southern quarter of the sky, overlapping with the region from which high-energy (>100TeV) neutrino events have been found. We characterize the parsec-scale radio properties of the jets and compare with the quasi-s…

observational astronomyActive galactic nucleigalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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AB Dor A VLBI images

2020

The fast rotator, pre-main sequence star AB Dor A is a strong and persistent radio emitter. The extraordinary coronal flaring activity is thought to be the origin of compact radio emission and other associated phenomena, such as large slingshot prominences. We aim to investigate the radio emission mechanism and the milliarcsecond radio structure around AB Dor A. We performed phase-referenced VLBI observations at 22.3GHz, 8.4GHz, and 1.4GHz over more than one decade using the Australian VLBI array. Our 8.4GHz images show a double core-halo morphology, similar at all epochs, with emission extending at heights between 5 and 18 stellar radii. Furthermore, the sequence of the 8.4GHz maps shows a…

observational astronomyPre main sequence starsAstrophysics and AstronomyStellar AstronomyPhysicsNatural SciencesPre-main sequence starsVery long baseline interferometry
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TANAMI monitoring of Centaurus A.

2015

Centaurus A (Cen A) is the closest radio-loud active galactic nucleus. Very Long Baseline Interferometry (VLBI) enables us to study the spectral and kinematic behavior of the radio jet-counterjet system on milliarcsecond scales, providing essential information for jet emission and propagation models. In the framework of the TANAMI monitoring, we investigate the kinematics and complex structure of Cen A on subparsec scales. We have been studying the evolution of the central parsec jet structure of Cen A for over 3.5-years. The proper motion analysis of individual jet components allows us to constrain jet formation and propagation and to test the proposed correlation of increased high-energy …

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsRadio galaxiesAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesGalaxiesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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The gNLS1 galaxy PKS 2004-447. VLBI images

2016

Gamma-ray-detected radio-loud narrow-line Seyfert 1 (g-NLS1) galaxies constitute a small but interesting sample of the g-ray-loud AGN. The radio-loudest g-NLS1 known, PKS 2004-447, is located in the southern hemisphere and is monitored in the radio regime by the multiwavelength monitoring programme TANAMI. We aim for the first detailed study of the radio morphology and long-term radio spectral evolution of PKS 2004-447, which are essential for understanding the diversity of the radio properties of g-NLS1s. The TANAMI VLBI monitoring program uses the Australian Long Baseline Array (LBA) and telescopes in Antarctica, Chile, New Zealand, and South Africa to monitor the jets of radio-loud activ…

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsRadio galaxiesAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesGalaxiesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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Catching the radio flare in CTA 102

2013

Very Long Baseline Interferometry (VLBI) observations can resolve the radio structure of active galactic nuclei (AGN) and provide estimates of the structural and kinematic characteristics on parsec-scales in their jets. The changes in the kinematics of the observed jet features can be used to study the physical conditions in the innermost regions of these sources. We performed multifrequency multiepoch Very Long Baseline Array (VLBA) observations of the blazar CTA102 during its 2006 radio flare, the strongest ever reported for this source. These observations provide an excellent opportunity to investigate the evolution of the physical properties of blazars, especially during these flaring e…

observational astronomygalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsStellar AstronomyPhysicsNatural SciencesQuasarsVery long baseline interferometry
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Pankin pääomarakenne ja varainhankinta nykyisessä ja tulevassa pankkisääntelyssä

2017

Tämä tutkielma kokoaa yhteen pankkeja nykyisin velvoittavat pääomien määrään ja maksuvalmiuteen sekä rahoitukseen liittyvät sääntelyt. Tutkielman tavoitteena on saada vastaus kysymykseen: Miten pankin tulee huomioida pankkisääntely pääoman ja varainhankinnan rakenteessaan? Tutkielman alussa esitellään pankkitoimintaa yleisesti ja siihen liittyviä optimointiongelmia. Pankkien kannalta optimaalinen pääomarakenne poikkeaa sosiaalisesti optimaalisesta ja tätä varten pankkisääntelyä tarvitaan. Optimaalisimman tason määrittely on haastavaa, mutta sen on arvioitu olevan 15-20 % tasolla. Pääomarakenteella on vaikutusta pankin tuottavuuteen ja menestymisen mahdollisuuksiin. Pankkeja voidaan säännell…

pääomapankitMinimum Requirement for Own Funds and Eligible Liabilities (MREL)pankkisääntelyoikeudellinen sääntelyBasel IIITapaustutkimusmaksuvalmiusvalvontavarainhankintaLiquidity Coverage Ratio (LCR)Net Stable Funding Ratio (NSFR)
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Modelling Recurrent Events for Improving Online Change Detection

2016

The task of online change point detection in sensor data streams is often complicated due to presence of noise that can be mistaken for real changes and therefore affecting performance of change detectors. Most of the existing change detection methods assume that changes are independent from each other and occur at random in time. In this paper we study how performance of detectors can be improved in case of recurrent changes. We analytically demonstrate under which conditions and for how long recurrence information is useful for improving the detection accuracy. We propose a simple computationally efficient message passing procedure for calculating a predictive probability distribution of …

ta113noiseComputer scienceData stream miningMessage passingDetectordata streamsonline change detection02 engineering and technologycomputer.software_genreTask (computing)recurrent eventschange points020204 information systems0202 electrical engineering electronic engineering information engineeringProbability distribution020201 artificial intelligence & image processingNoise (video)Data miningBaseline (configuration management)computerChange detectionProceedings of the 2016 SIAM International Conference on Data Mining
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