Search results for " observation"

showing 10 items of 441 documents

A precise photometric ratio via laser excitation of the sodium layer - I. One-photon excitation using 342.78 nm light

2020

The largest uncertainty on measurements of dark energy using type Ia supernovae is presently due to systematics from photometry; specifically to the relative uncertainty on photometry as a function of wavelength in the optical spectrum. We show that a precise constraint on relative photometry between the visible and near-infrared can be achieved in upcoming surveys (such as in LSST at the Vera C. Rubin Observatory) via a mountaintop-located laser source tuned to the 342.78 nm vacuum excitation wavelength of neutral sodium atoms. Using a high-power (500 W) laser modified from laser guide star studies, this excitation will produce an artificial star (which we term a "laser photometric ratio s…

PhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicslaw.inventionPhotometry (optics)techniques: photometricOpticslawAstrophysics::Solar and Stellar Astrophysicsdark energyInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsPhysicsbusiness.industrymethods:observationalAstrophysics::Instrumentation and Methods for AstrophysicsSodium layerAstronomy and AstrophysicstelescopesLaser[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]instrumentation: miscellaneousWavelengthLaser guide starSpace and Planetary Science[SDU]Sciences of the Universe [physics]instrumentation:miscellaneousmethods: observationalbusinesstechniques:photometricAstrophysics - Instrumentation and Methods for AstrophysicsExcitationVisible spectrumAstrophysics - Cosmology and Nongalactic Astrophysics
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Prolonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

2019

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim$20.1 (3300-10500 $\require{mediawiki-texvc} \AA$). The optical emission was variable on timescales from hundreds to thousands of seconds. The spectrum showed prominent emission lines with variable profiles at different epochs. Simultaneous XMM-Newton and NuSTAR observations revealed a bimodal distribution of the X-ray count rates on timescales as short as tens of seconds, as well as sporadic flaring activity. The average broad-band (0.3-79 keV) spectrum was adequately described by an absorbed power law model with…

PhotonX-rays: BinarieAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstrophysicsMethods: Data analysiAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesLuminosityAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaPulsarMethods: Observational0103 physical sciencesEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsStars: neutronX-rays: Individuals: CXOU J110926.4-650224Neutron star13. Climate actionSpace and Planetary ScienceMagnitude (astronomy)Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space Telescope
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IGUALDADE DE GÊNERO E ANÁLISE DA COMUNICAÇÃO MOTORA NAS TAREFAS DE EDUCAÇÃO FÍSICA

2019

Resumen El presente artículo analiza las tareas motrices propuestas en el ámbito de la Educación Física, tanto por el maestro como en el juego libre, desde una perspectiva de género. A partir de una observación participante se obtienen las tareas propuestas en las sesiones de Educación Física de una escuela en la localidad de Meliana, en la provincia de Valencia (España). Se constatan 134 tareas motrices que se analizan y contextualizan en el marco educativo. Los resultados muestran que se tiende a impulsar un cierto modelo de comportamiento común cuando el docente ejerce mayor directividad. En cambio, cuando el profesor ofrece libertad para escoger, se tienden a reproducir los estereotipos…

Physical activityAtividade físicaPerspective (graphical)Participant observationEducational frameworkIdentidade de gêneroEducationPhysical educationFree playGender identityActividad físicaEducação FísicaPhysical educationEducación FísicaIdentidad de géneroPsychologySocial psychology
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X-ray emitting hot plasma in solar active regions observed by the SphinX spectrometer

2012

Aims. The detection of very hot plasma in the quiescent corona is important for diagnosing heating mechanisms. The presence and the amount of such hot plasma is currently debated. The SphinX instrument on-board the CORONAS-PHOTON mission is sensitive to X-ray emission of energies well above 1 keV and provides the opportunity to detect the hot plasma component. Methods. We analysed the X-ray spectra of the solar corona collected by the SphinX spectrometer in May 2009 (when two active regions were present). We modelled the spectrum extracted from the whole Sun over a time window of 17 days in the 1.34− 7k eV energy band by adopting the latest release of the APED database. Results. The SphinX …

Physics010504 meteorology & atmospheric sciencesSpectrometerX-rayBremsstrahlungAstronomy and AstrophysicsPlasmaAstrophysics01 natural sciencesCoronaSpectral lineSun: corona methods: observational techniques: spectroscopicStars13. Climate actionSpace and Planetary Science0103 physical sciencesCalibration010303 astronomy & astrophysics0105 earth and related environmental sciencesAstronomy & Astrophysics
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Direct observation of theBa114→Xe110→Te106→Sn102tripleα-decay chain using position and time correlations

2016

The triple $\ensuremath{\alpha}$-decay chain $^{114}\mathrm{Ba}\ensuremath{\rightarrow}^{110}\mathrm{Xe}\ensuremath{\rightarrow}^{106}\mathrm{Te}\ensuremath{\rightarrow}^{102}\mathrm{Sn}$ has been directly observed for the first time, following the $^{58}\mathrm{Ni}(^{58}\mathrm{Ni},2n)$ reaction. Implantation of $^{114}\mathrm{Ba}$ nuclei into a double-sided silicon-strip detector has allowed their $\ensuremath{\alpha}$ decays to be correlated in position and time with the $\ensuremath{\alpha}$ decays of the daughter $(^{110}\mathrm{Xe})$ and granddaughter $(^{106}\mathrm{Te})$ nuclei. In total, 17 events have been assigned to the $^{114}\mathrm{Ba}\ensuremath{\rightarrow}^{110}\mathrm{Xe}…

PhysicsCluster decay010308 nuclear & particles physics0103 physical sciencesDirect observationDecay chainAtomic physics010306 general physics01 natural sciencesRecoil separatorEnergy (signal processing)Physical Review C
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The Chandra COSMOS Survey, I: Overview and Point Source Catalog

2009

The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra} program that has imaged the central 0.5 sq.deg of the COSMOS field (centered at 10h, +02deg) with an effective exposure of ~160ksec, and an outer 0.4sq.deg. area with an effective exposure of ~80ksec. The limiting source detection depths are 1.9e-16 erg cm(-2) s(-1) in the Soft (0.5-2 keV) band, 7.3e(-16) erg cm^-2 s^-1 in the Hard (2-10 keV) band, and 5.7e(-16) erg cm(-2) s(-1) in the Full (0.5-10 keV) band. Here we describe the strategy, design and execution of the C-COSMOS survey, and present the catalog of 1761 point sources detected at a probability of being spurious of <2e(-5) (1655 in the Full, 1340 in the Soft, and…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)biologyInfraredPoint sourceFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLimitingbiology.organism_classificationAcisSpace and Planetary SciencePoint (geometry)Astrophysics - High Energy Astrophysical Phenomenacatalogs – cosmology: observations – galaxies: evolution – quasars: general – surveys – X-rays: generalCosmosAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for pulsations at high radio frequencies from accreting millisecond X-ray pulsars in quiescence

2010

It is commonly believed that millisecond radio pulsars have been spun up by transfer of matter and angular momentum from a low-mass companion during an X-ray active mass transfer phase. A subclass of low-mass X-ray binaries is that of the accreting millisecond X-ray pulsars, transient systems that show periods of X-ray quiescence during which radio emission could switch on. The aim of this work is to search for millisecond pulsations from three accreting millisecond X-ray pulsars, XTE J1751-305, XTE J1814-338, and SAX J1808.4-3658, observed during their quiescent X-ray phases at high radio frequencies (5 - 8 GHz) in order to overcome the problem of the free-free absorption due to the matter…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLuminosityInterstellar medium85-05pulsars general methods data analysis methods observational stars neutron X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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Time reversal violation for entangled neutral mesons

2013

A direct evidence for Time Reversal Violation (TRV) means an experiment that, considered by itself, clearly shows TRV independent of, and unconnected to, the results for CP Violation. No existing result before the recent BABAR experiment with entangled neutral B mesons had demonstrated TRV in this sense. There is a unique solution for the test of TRV with unstable particles thanks to the Einstein-Podolsky-Rosen (EPR) Entanglement between the two neutral mesons in B, and φ, Factories. The two quantum effects of the decays as filtering measurements of the meson states and the transfer of information of the first decay to the still living partner allow performing a genuine TRV asymmetry with t…

PhysicsHistoryParticle physicsMesonmedia_common.quotation_subjectDirect observationTime evolutionBaBar experimentQuantum entanglementAsymmetryComputer Science ApplicationsEducationsymbols.namesakesymbolsCP violationHigh Energy Physics::ExperimentB mesonEPR paradoxmedia_commonAIP Conference Proceedings
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Novel T-violation observable open to any decay channel at meson factories

2015

Two genuine Quantum phenomena: Entanglement and Filtering Measurement are at the origin of the first direct observation of Time-Reversal-Violation in the time evolution of the B neutral meson system by BaBar. The used meson transitions are directly connected to semileptonic and CP-eigenstate decay channels. We analyse the possibility of extending the observable asymmetries to more decay channels. We propose an alternative T-Violation Asymmetry in the meson factories which allows its opening to any pair of decay channels. The new asymmetry needs also the measurement of the time dependent total survival probability of the initial tagged states. By combining several asymmetries these total sur…

PhysicsHistoryParticle physicsMesonmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyEta mesonTime evolutionDirect observationMacroscopic quantum phenomenaObservableQuantum entanglementAsymmetryComputer Science ApplicationsEducationNuclear physicsHigh Energy Physics::Experimentmedia_commonCommunication channelProceedings of Proceedings of the Corfu Summer Institute 2014 — PoS(CORFU2014)
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On the identification of celestial γ-ray sources

1978

THE observations from COS B have provided a new and more detailed picture of the high energy γ-ray emission from the Galaxy. We discuss here the first catalogue with 13 localised sources which has been compiled1,2 and how the list should lengthen in the near future, as the data analysis progresses.

PhysicsIdentification (information)High energySatellite observationMultidisciplinaryGamma ray spectrometerAstronomyQuasarAstrophysicsGamma-ray astronomyAstronomical spectroscopyGalaxyNature
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