Search results for "RAYS"

showing 10 items of 1136 documents

Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina-Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia-the Australian Research Council; Brazil…

interaction: modelPhysics::Instrumentation and DetectorsAstronomyHadronGeneral Physics and AstronomyUltra-high energy cosmic rays muons properties hadronic models01 natural sciencescosmic ray; particle interaction; astroparticle detectorsAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ironsurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]cosmic rayPhysics4. EducationPhysicsSettore FIS/01 - Fisica Sperimentalemeasured [fluctuation]model [interaction]Astrophysics::Instrumentation and Methods for Astrophysicsmodel: hadronicfluctuation: measured3. Good healthAugerobservatoryparticle interactionSciences exactes et naturellesatmosphere [showers]model [particle]airCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesCosmic raydetector: fluorescenceNuclear physicsastroparticle detectorscosmic raysmuon0103 physical sciencescalorimeterddc:53014. Life underwatercosmic radiation: UHEHigh Energy Physicsdistribution functionelectromagnetic component010306 general physicsAstrophysiquePierre Auger Observatoryfluorescence [detector]Muonshowers: atmospherehep-exdetector: surfacewater [Cherenkov counter]particle: modelSmall deviationsFísicaASTROFÍSICAAir showerExperimental High Energy PhysicsElementary Particles and Fieldshadronic [model]High Energy Physics::Experiment
researchProduct

X-Ray Nanotomography of Individual Pulp Fibre Bonds Reveals the Effect of Wall Thickness on Contact Area

2019

Fibre bonds play an essential role in various properties of paper. Much research has focused on their strength, but the determination of the actual contact area also provides a challenge. Many of the research methods rely on optical tools, which are restricted by the wavelength of light that is utilised. Novel X-ray computed tomography devices utilise X-rays in studying the inner structure of materials, and surpass the optical methods in terms of resolution, allowing detection of even smaller details and variations in distance between the fibres in the bond intersection area. X-ray nanotomography was used to image 26 individual cellulose fibre bonds made of springwood and summerwood fibres …

kuvantaminenröntgenkuvauslcsh:RX-rayslcsh:Medicinelcsh:Qlcsh:ScienceCIBM-PCArticleimaging techniquesbiomateriaalit
researchProduct

Estudio de la adaptación a estrés por etanol en cepas de Saccharomyces cerevisiae

2016

Los mecanismos de tolerancia a etanol han sido ampliamente estudiados en la levadura Saccharomyces cerevisiae debido a su importancia en el sector industrial de bebidas fermentadas y obtención de biocombustibles, siendo las cepas de laboratorio las más utilizadas en los estudios experimentales. A pesar del gran número de estudios llevados a cabo, nuestra comprensión de la respuesta transcripcional y fisiológica al etanol continúa siendo limitada debido al uso de cepas no adecuadas para este fin y la gran disparidad en las condiciones utilizadas. Además se ha dejado de lado el estudio de ciertas rutas de respuesta a estrés en levaduras, como la respuesta a proteínas desplegadas (UPR), cuya a…

levadurasSaccharomycesetanolUNESCO::CIENCIAS DE LA VIDAUPRmicroarrays:CIENCIAS DE LA VIDA [UNESCO]
researchProduct

Resolving the Fe XXV triplet with Chandra in Centaurus X-3

2005

We present the results of a 45 ks Chandra observation of the high-mass X-ray binary Cen X-3 at orbital phases between 0.13 and 0.40 (in the eclipse post-egress phases). Here we concentrate on the study of discrete features in the energy spectrum at energies between 6 and 7 keV, that is, on the iron K alpha line region, using the High Energy Transmission Grating Spectrometer (HETGS) on board the Chandra satellite. We clearly see a K alpha neutral iron line at similar to 6.40 keV and were able to distinguish the three lines of the Fe xxv triplet at 6.61, 6.67, and 6.72 keV, with equivalent widths of 6, 9, and 5 eV, respectively. The equivalent width of the Ka neutral iron line is 13 eV, an or…

line : formationline : identificationpulsars : individual (Centaurus X-3)X-rays : binarieformation; line : identification; pulsars : individual (Centaurus X-3); X-rays : binaries; X-rays : general [line]X-rays : general
researchProduct

Long-term monitoring of the TeV emission from Mrk 421 with the ARGO-YBJ experiment

2011

ARGO-YBJ is an air shower detector array with a fully covered layer of resistive plate chambers. It is operated with a high duty cycle and a large field of view. It continuously monitors the northern sky at energies above 0.3 TeV. In this paper, we report a long-term monitoring of Mrk 421 over the period from 2007 November to 2010 February. This source was observed by the satellite-borne experiments Rossi X-ray Timing Explorer and Swift in the X-ray band. Mrk 421 was especially active in the first half of 2008. Many flares are observed in both X-ray and gamma-ray bands simultaneously. The gamma-ray flux observed by ARGO-YBJ has a clear correlation with the X-ray flux. No lag between the X-r…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaOggetti di tipo BL LacertaeFOS: Physical sciencesFluxAstrophysics01 natural sciences7. Clean energyindividual (Markarian 421) [BL Lacertae objects]Spectral lineGamma-rays Markarian 421 BL Lacertae Resistive Plate Chamberslaw.inventionlaw0103 physical sciencesRadiative transfer010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsMarkarian 421Settore FIS/01 - Fisica SperimentaleAstronomy and Astrophysicsgeneral [gamma ray]Synchrotron3. Good healthAir shower13. Climate actionSpace and Planetary ScienceDuty cycleSkyRaggi gammaSpectral energy distributionAstrophysics - High Energy Astrophysical Phenomena
researchProduct

Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006

2018

We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN. We extract the NuSTAR spectra from a few regions along the non-thermal limbs and jointly analyze them with the XMM-Newton spectra and the radio data. The broad-band radio/X-ray spectra can be well described with a synchrotron emission model from a single population of CR electrons with a power law energy distribution and an exponential cutoff. The power law index of the electron particle distribution function (PDF) is ~1.88-1.95 for both the NE and SW l…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryPower lawSpectral linecosmic rays0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumeducation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonISM: supernova remnantsacceleration of particlesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsshock wavesAstronomy and Astrophysicradiation mechanisms: non-thermalX-rays: ISMMagnetic fieldSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
researchProduct

Discovery of slow X-ray pulsations in the high-mass X-ray binary 4U 2206+54

2008

Context. The source 4U 2206+54 is one of the most enigmatic high-mass X-ray binaries. In spite of intensive searches, X-ray pul- sations have not been detected in the time range 10−3–103 s. A cyclotron line at ∼30 keV has been suggested by various authors but never detected with significance. The stellar wind of the optical companion is abnormally slow. The orbital period, initially reported to be 9.6 days, disappeared and a new periodicity of 19.25 days emerged. Aims. The main objective of our RXTE monitoring of 4U 2206+54 is to study the X-ray orbital variability of the spectral and timing parameters. The new long and uninterrupted RXTE observations allow us to search for long (∼1 h) puls…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenapulsars : general [Stars]X-ray binaryFOS: Physical sciencesOrbital eccentricityAstrophysicsAstrophysicsStars : early-type; Stars : emission-line Be; Stars : binaries : close; X-rays : binaries; Stars : pulsars : generalLuminosityearly-type [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XAstrophysics::Solar and Stellar AstrophysicsEccentricity (behavior)binaries : close [Stars]media_commonLine (formation)PhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsOrbital periodLight curveNeutron starSpace and Planetary Scienceemission-line Be [Stars]binaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
researchProduct

The subway tunneling technique for distal shunt catheter insertion.

2019

Dear Editor,We read with interest the article by Osman et al. titled ‘Trocar assisted distal shunt tube insertion with intra-operative X-Ray confirmation’. The authors purpose their technique to pl...

medicine.medical_specialtyCatheter insertionHydrocephalubusiness.industryX-RaysGeneral MedicineSurgical InstrumentsSurgical InstrumentVentriculoperitoneal ShuntSurgeryShunt (medical)medicineHumansSurgeryRailroadNeurology (clinical)businessRailroadsHumanHydrocephalusBritish journal of neurosurgery
researchProduct

S2k guidelines for the treatment of psoriasis in children and adolescents - Short version part 1.

2019

The present guidelines are aimed at residents and board-certified physicians in the fields of dermatology, pediatrics, pediatric dermatology and pediatric rheumatology as well as policymakers and insurance funds. They were developed by dermatologists and pediatric dermatologists in collaboration with pediatric rheumatologists using a formal consensus process (S2k). The guidelines highlight topics such as disease severity, quality of life, treatment goals as well as problems associated with off-label drug therapy in children. Trigger factors and diagnostic aspects are discussed. The primary focus is on the various topical, systemic and UV-based treatment options available and includes recomm…

medicine.medical_specialtyConsensusAdolescentUltraviolet RaysAdministration TopicalMEDLINEDiseaseComorbidityDermatologySeverity of Illness Index030207 dermatology & venereal diseases03 medical and health sciencesPsoriatic arthritis0302 clinical medicineQuality of life (healthcare)PharmacotherapyRheumatologyPsoriasisSeverity of illnessmedicineHumansPsoriasisIntensive care medicineChildbusiness.industryArthritis PsoriaticInfant NewbornInfantOff-Label Usemedicine.diseaseChild PreschoolPractice Guidelines as TopicQuality of LifebusinessGuttate psoriasisJournal der Deutschen Dermatologischen Gesellschaft = Journal of the German Society of Dermatology : JDDGReferences
researchProduct

Study of the interocclusal distortion in impressions taken with different types of closed-mouth trays and two types of impression materials

2010

The aim of this study was to compare different types of impression trays for the closed-mouth impression technique, using two different types of impression material. For this study, five different types of impression trays were used with two different types of impression materials, one of addition silicone and the other of polyether. We designed a model used for taking the impressions and for measuring interocclusal distortion. The results obtained show that the impression trays COE (GC (R) GC America INC. Alsip) and Premier (Premier (R), Premier Dental Products Co. Canada) show a lesser degree of interocclusal distortion when taking closed-mouth impressions. In terms of impression material…

medicine.medical_specialtyDental Impression TechniqueComputer scienceClosed-Mouth ImpressionsOdontologíaImpression traysDental OcclusionCirugíaDistortionDentistry Oral Surgery & MedicinemedicineDental Impression TechniqueDual-Arch ImpressionsGeneral DentistryOrthodonticsDental occlusionDental Impression MaterialsPolyetherEquipment Design:CIENCIAS MÉDICAS [UNESCO]Closed mouthSurgeryImpressionImpression TraysTrayOtorhinolaryngologyUNESCO::CIENCIAS MÉDICASDental impression materialSurgeryInterocclusal DistortionMedicina Oral Patología Oral y Cirugia Bucal
researchProduct