Search results for "COPI"

showing 10 items of 2618 documents

Chemometric Tools to Point Out Benchmarks and Chromophores in Pigments through Spectroscopic Data Analyses

2021

Spectral preprocessing data and chemometric tools are analytical methods widely applied in several scientific contexts i.e., in archaeometric applications. A systematic classification of natural powdered pigments of organic and inorganic nature through Principal Component Analysis with a multi-instruments spectroscopic study is presented here. The methodology allows the access to elementary and molecular unique benchmarks to guide and speed up the identification of an unknown pigment and its recipe. This study is conducted on a set of 48 powdered pigments and tested on a real-case sample from the wall painting in S. Maria Delle Palate di Tusa (Messina, Italy). Four spectroscopic techniques …

ancient pigmentsspectroscopic techniquesOrganic ChemistryPharmaceutical Scienceancient pigments; spectroscopic techniques; chemometrics discrimination; elemental and molecular benchmarksArticlechemometrics discriminationAnalytical Chemistryelemental and molecular benchmarksQD241-441Chemistry (miscellaneous)Drug DiscoveryMolecular MedicinePhysical and Theoretical ChemistryMolecules; Volume 27; Issue 1; Pages: 163
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Antennal sensilla ofNeomysis integer (leach)

1978

The most frequent type of the hair sensilla on the antennae ofNeomysis integer is investigated by electron microscopic methods. The cellular properties of the sensilla are compared with those of other arthropods in order to detect possible homologies.

animal structuresnervous systemfungiBiophysicssense organsCell BiologyPlant ScienceGeneral Medicinerespiratory systemBiologyElectron microscopicInteger (computer science)Protoplasma
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Impiego della lmax del vino nel visibile come indicatore della presenza di antociani copigmentati

2007

antociani copigmenti spettrometriaSettore AGR/15 - Scienze E Tecnologie Alimentari
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A clampless and sutureless aortic anastomosis technique using an endograft connector for aortoiliac occlusive disease in which the aorta cannot be cl…

2012

Bypass surgery in aortoiliac or aortofemoral occlusive disease can be technically demanding and hazardous due to huge calcifications and/or patient co-morbidities. We report about mid-term results of a telescoping sutureless aortic anastomosis technique using endografts as connectors to address such challenging situations. This is a single-center experience (2004–2011) in seven patients (63 ± 6 years) requiring aortoiliac (three) or aortofemoral (four) bypass surgery. In six cases, an aortic stent graft was telescoped into the infrarenal aorta and partly deployed within the aorta and partly outside the aorta. In the first case, a bifurcated stent graft was deployed and the iliac legs were p…

aortoiliac occlusive diseasecalcified aortacross-clampingmid-term resultsSettore MED/22 - Chirurgia Vascolareclampless-telescoping anastomosi
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Análisis espectroscópico de fragmentos cometarios y asteroidales a su entrada en la atmósfera terrestre.

2002

En la presente tesis se analiza el origen y composición de la materia interplanetaria a partir de una perspectiva nueva basada en el estudio de los fenómenos luminosos que producen estas partículas a su entrada a la atmósfera terrestre, llamados meteoros. Estas partículas, procedentes mayoritariamente de la degradación de las superficies de cometas y asteroides, cuando se hayan en órbita solar se denominan genéricamente meteoroides. Dependiendo de la geometría del encuentro con la Tierra los meteoroides alcanzan la atmósfera a velocidades comprendidas en el rango de 11 a 73 km/s. A estas velocidades a alturas de entre 120 y 70 km. la densidad atmosférica es suficiente para que las colisione…

asteroides52Matemáticasespectroscopiameteoroides y abundancias químicas.calculo de orbitascometas
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HADES RV programme with HARPS-N at TNG: XII. The abundance signature of M dwarf stars with planets

2020

[Context] Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing.

astro-ph.SRStellar massMetallicityFOS: Physical sciencesTechniques: spectroscopicStars: late-typeAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesspectroscopic [Techniques]Settore FIS/05 - Astronomia E AstrofisicaPrimary (astronomy)PlanetAbundance (ecology)0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsEarth and Planetary Astrophysics (astro-ph.EP)Physics010308 nuclear & particles physicsStars: abundancesGiant planetAstronomy and Astrophysicsastro-ph.SR; astro-ph.SR; astro-ph.EPRadial velocityStarsPlanetary systemsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Scienceabundances [Stars]late-type [Stars]astro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
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Multi-wavelength surveys: object detectability an nir luminosity function of galaxies

2011

El estudio de la evolución de la FL se extendió al rango infrarrojo, en las bandas en reposo J y H, hasta redshift 3.5. Este fue el resutlado del análisis de tres catálogos públicos desde los proyectos MUSYC, FIRES y FIREWORKS. El análisis nos permitió medir por primera vez la FL en la banda H de reposo de galaxias de campo en el rango de redshift z ¿ [1.5,3.5]; al mismo tiempo, el mayor volumen nos permitió mejorar de manera significativa la medida del extremo brillante de la FL. Desde el punto de vista espectroscópico, desarrollamos un método novedoso para el análisis de espectros con baja razón señal-ruido, parecido a los utilizados en el análisis de datos de rayos X. El método consiste …

astronomíaastrofísicagalaxiasespectroscopia astrofísicaUNESCO::ASTRONOMÍA Y ASTROFÍSICA:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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About the link between the detailed description of transitions in a ion and the average-ion models.

2009

We study the link which exists between microscopic (detailed) models for the evolution of the electronic configurations in a population of ions and the macroscopic (average ion) models. Rigorous asymptotics are presented in situations where they exist (large temperature; almost empty or almost full shells), and numerical simulations are presented.

average ion modelmicroscopic modelrigorous asymptoticcomparison of solutions
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Propiedades psicométricas del cuestionario de afronta¬miento al estrés para pacientes oncológicos (CAEPO)

2017

Los objetivos del estudio fueron: 1) analizar la estructura factorial de la escala CAEPO mediante análisis factorial exploratorio y confirmatorio; 2) estimar la consistencia interna de los factores; 3) describir la distribución de los factores; 4) analizar las diferencias de medias de las estrategias de afrontamiento entre hombres y mujeres. El Cuestionario de Afrontamiento al Estrés para Pacientes Oncológicos (CAEPO) de González (2004) fue aplicado a 148 pacientes oncológicos. Se sugiere reducir la escala a 35 ítems. Se encontró una estructura de cuatro factores correlacionados con consistencias internas de adecuadas a altas. La distribución de los factores se ajustó a una curva normal y n…

avoidanceAfrontamiento activolcsh:BF1-990ruminaterumiaciónlcsh:Neoplasms. Tumors. Oncology. Including cancer and carcinogenslcsh:RC254-282cáncer.Active copingClinical Psychologylcsh:PsychologyOncologycancer.pasividadevitaciónpassiveness
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