Search results for "COPE"

showing 10 items of 3215 documents

Search for high energy cosmic muon neutrinos from variable gamma-ray sources and time calibration of the optical modules of the ANTARES telescope

2015

325 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear de la Universidad de Valencia y del Instituto de Física Corpuscular (IFIC).

ANTAREStelescopios de neutrinosAGNsAstrophysics::High Energy Astrophysical PhenomenablazarsFísica experimental de Altas Energíasneutrino telescopesAstrophysics::Instrumentation and Methods for AstrophysicsneutrinosNebulosa del CangrejoXRBsX-ray binaries:FÍSICA::Física de altas energías [UNESCO]UNESCO::FÍSICA::Física de altas energíasCrab Pulsar Wind Nebulabinarias de rayos X
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Esigenze conservative e prestazioni tecnologiche: linee guida per la copertura della Domus ellenistica-romana di Taormina

2005

AREE ARCHEOLOGICHE SISTEMI DI PROTEZIONI COPERTURE
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Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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Study of the electronic and atomic structure of thermally treated SrTiO3(110) surfaces

2003

The electronic structure of heated SrTiO3(110) surfaces was investigated with metastable impact electron spectroscopy and ultraviolet photoelectron spectroscopy (He(I). Scanning tunnelling microscopy and atomic force microscopy (AFM) were used to study the topology of the surface. The crystals were heated up to 1000 °C under reducing conditions in ultrahigh vacuum or under oxidizing conditions in synthetic air for 1 h, respectively. Under both conditions microfacetting of the surface is observed. The experimental results are compared with ab initio Hartree-Fock calculations, also presented here, carried out for both ideal and reconstructed SrTiO 3(110) surfaces. The results give direct evid…

Ab initioAnalytical chemistrySurfaces and InterfacesGeneral ChemistryElectronic structureCondensed Matter PhysicsElectron spectroscopySurfaces Coatings and Filmslaw.inventionCondensed Matter::Materials Sciencechemistry.chemical_compoundchemistryAb initio quantum chemistry methodslawMicroscopyMaterials ChemistryStrontium titanateAtomic physicsScanning tunneling microscopeUltraviolet photoelectron spectroscopySurface and Interface Analysis
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Analysis of the morphology and composition of tooth apices apicectomized using three different ablation techniques.

2011

Objectives: To investigate apicectomies performed using burs, a CO2 laser or an Er:YAG laser and to evaluate the following aspects: morphology of apicectomized surfaces, presence of failures at the dentin/obturation material interface (marginal fit) of the apical portions of the root canals, and the proportions of chemical elements in the apicectomized surfaces. Study design: Twenty-four teeth were divided into three groups of eight and each group underwent apicectomy by one of three different ablation techniques: bur, CO2 laser or Er:YAG laser. The morphology of the apicectomized surfaces was then analyzed using scanning electron microscopy and their chemical composition was analyzed by en…

Ablation TechniquesAdultMaterials scienceScanning electron microscopeAblation Techniquesmedicine.medical_treatmentEnergy-dispersive X-ray spectroscopyDentistryLasers Solid-StateCiências da Saúde Outras ciências médicasApicectomylaw.inventionTooth ApexlawDentinmedicineHumansHealth sciences Other medical sciencesGeneral Dentistrybusiness.industrymicroanálise por EDS:Other medical sciences [Medical and Health sciences]Tooth ApexMiddle Aged:CIENCIAS MÉDICAS [UNESCO]AblationLasermedicine.anatomical_structureOtorhinolaryngologyUNESCO::CIENCIAS MÉDICASLasers GasSurgeryMEV- Microscopia Eletrônica de Varreduar:Outras ciências médicas [Ciências médicas e da saúde]businessBiomedical engineeringMedicina oral, patologia oral y cirugia bucal
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The large trans-Neptunian object 2002 TC 302 from combined stellar occultation, photometry, and astrometry data

2020

All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Mazzei, L.; Mikuz, H.; Skvarc, J.; Ciabattari, F.; Lavalade, F. Scarfi, G.; Mari, J. M.; Conjat, M.; Sposetti, S.; Bachini, M.; Succi, G.; Mancini, F.; Alighieri, M.; Dal Canto, E.; Masucci, M.; Vara-Lubiano, M.; Gutiérrez, P. J.; Desmars, J.; Lecacheux, J.; Vieira-Martins, R.; Camargo, J. I. B.; Assafin, M.; Colas, F.; Beisker, W.; Behrend, R.; Mueller, T. G.; Meza, E.; Gomes-Junior, A. R.; Roques, F.; Vachier, F.; Mottola, S.; Hellmich, S.; Campo …

Absolute magnitude010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsKuiper belt objects: individual: 2002 TC30201 natural sciencesOccultationlaw.inventionTelescopePhotometry (optics)lawGeometric albedoFísica Aplicada0103 physical sciencesTrans-Neptunian object010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Earth and Planetary Astrophysics (astro-ph.EP)photometric [Techniques]Astronomy and Astrophysicsgeneral [Kuiper belt]Astrometryindividual: 2002 TC302 [Kuiper belt objects]AstrometryAstrometry; Kuiper belt objects: individual: 2002 TC302; Kuiper belt: general; Occultations; Techniques: photometricLight curveSpace and Planetary Science[SDU]Sciences of the Universe [physics]Kuiper belt: generalOccultations[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Techniques: photometricAstrophysics - Earth and Planetary AstrophysicsAstronomy & Astrophysics
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Hybrid layers of etch-and-rinse versus self-etching adhesive systems.

2010

Objective: To evaluate the effectiveness in the formation of resin tags, adhesive lateral branches and hybrid layers of five adhesive systems, when bonding to dentine. Material and Methods: Flat dentin surfaces from 25 molars were bonded with several adhesive systems according to the manufacturers? instructions. Composite build-ups were constructed incrementally with Tetric Ceram. The Specimens were sectioned parallel to the long axis. One section was treated with phosphoric acid and sodium hypochlorite in order to reveal the hybrid layer formation. The other section was stored in 30% hydrochloric acid to detect resin tags and adhesive lateral branch formation. Results: The two etch-and-rin…

Absorption of waterMaterials scienceScanning electron microscopeComposite numberDental Cementschemistry.chemical_compoundstomatognathic systemDentinmedicineHumansComposite materialGeneral DentistryBondingtechnology industry and agricultureDental Bonding:CIENCIAS MÉDICAS [UNESCO]medicine.anatomical_structureOtorhinolaryngologyPolymerizationchemistrySodium hypochloriteUNESCO::CIENCIAS MÉDICASDentinDental EtchingMicroscopy Electron ScanningSurgeryAdhesiveScanning electron microscopyLayer (electronics)Bonding Dentin Scanning electron microscopy
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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NuSTAR and NICER reveal IGR J17591-2342 as a new accreting millisecond X-ray pulsar

2018

We report the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsar IGR J17591-2342. Coherent X-ray pulsations around 527.4 Hz (1.9 ms) with a clear Doppler modulation were detected. This implies an orbital period of ∼8.8 h and a projected semi-major axis of ∼1.23 lt-s. With the binary mass function, we estimate a minimum companion mass of 0.42 M, obtained assuming a neutron star mass of 1.4[subscript ⊙] and an inclination angle lower than 60°, as suggested by the absence of eclipses or dips in the light curve of the source. The broad-band energy spectrum, obtained by combining NuS…

AccretionAstrophysics::High Energy Astrophysical Phenomenageneral [Pulsars]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linelaw.inventionTelescopeX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsarlow-mass [Stars]lawstars: low-mass0103 physical sciencesStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron Star Interior Composition Explorer010308 nuclear & particles physicsComputer Science::Information Retrievalaccretion disksneutron [Stars]Astronomy and AstrophysicsAstronomy and AstrophysicOrbital periodLight curveX-rays: binarieStars: neutronNeutron starPulsars: generalAccretion diskSpace and Planetary ScienceAccretion disksbinaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray pulsar
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Cast multibilayer films from polymerizable lipids

1987

Acrylate polymerPolymers and PlasticsChemistryScanning electron microscopeOrganic ChemistryAnalytical chemistryInorganic Chemistrychemistry.chemical_compoundMembranePhotopolymerChemical engineeringMaterials ChemistryIonic conductivityReverse osmosisUltraviolet radiationMacromolecules
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