Search results for " Planet"

showing 10 items of 5473 documents

New orbital ephemerides for the dipping source 4U 1323-619: Constraining the distance to the source

2016

4U 1323-619 is a low mass X-ray binary system that shows type I X-ray bursts and dips. The most accurate estimation of the orbital period is 2.941923(36) hrs and a distance from the source that is lower than 11 kpc has been proposed. We aim to obtain the orbital ephemeris, the orbital period of the system, as well as its derivative to compare the observed luminosity with that predicted by the theory of secular evolution. We took the advantage of about 26 years of X-ray data and grouped the selected observations when close in time. We folded the light curves and used the timing technique, obtaining 12 dip arrival times. We fit the delays of the dip arrival times both with a linear and a quad…

neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619 [stars]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesLuminositySettore FIS/05 - Astronomia E Astrofisica0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619Astronomy and AstrophysicsLight curveOrbital periodGalaxyNeutron starSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics - High Energy Astrophysical Phenomena
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Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

2006

We performed a timing analysis of the fastest accreting millisecond pulsar IGR J00291+5934 using RXTE data taken during the outburst of December 2004. We corrected the arrival times of all the events for the orbital (Doppler) effects and performed a timing analysis of the resulting phase delays. In this way we have the possibility to study, for the first time in this class of sources, the spin-up of a millisecond pulsar as a consequence of accretion torques during the X-ray outburst. The accretion torque gives us for the first time an independent estimate of the mass accretion rate onto the neutron star, which can be compared with the observed X-ray luminosity. We also report a revised valu…

neutron; stars : magnetic fields; pulsars : general; pulsars : individual : IGR J00291+5934; X-ray : binaries [accretion accretion disks; stars]X-rays : binariesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsaccretion accretion diskAstrophysicsX-ray : binariesBinary pulsarLuminositypulsars : individual : IGR J00291+5934symbols.namesakePulsarMillisecond pulsarAstrophysics::Solar and Stellar Astrophysicspulsars : individual (IGR J00291+5934)PhysicsAccretion (meteorology)general; pulsars : individual (IGR J00291+5934); stars : magnetic fields; stars : neutron; X-rays : binaries [pulsars]Astrophysics (astro-ph)pulsars : generalStatic timing analysisAstronomystars : magnetic fieldAstronomy and Astrophysicsstars : neutronNeutron starSpace and Planetary SciencesymbolsAstrophysics::Earth and Planetary AstrophysicsDoppler effectX-ray pulsar
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Description and phylogenetic relationships of a new species of treefrog of theOsteocephalus buckleyispecies group (Anura: Hylidae)

2020

The Osteocephalus buckleyi species group is widely distributed in primary and secondary forests of the Amazon Basin and Guiana Region. Based on integrative analysis, including morphological and genetic data, we estimate the phylogenetic relationships and species boundaries among populations of the Osteocephalus buckleyi group from the Ecuadorian Amazon, focusing on the O. verruciger-O. cannatellai species complex. Our results uncovered the existence of one confirmed candidate species from Sangay National Park and one unconfirmed candidate species. Here, we describe the new species which is morphologically and ecologically distinct from other Osteocephalus species. The new species is unusual…

new species0106 biological sciencesecuadorGlobal and Planetary ChangeOsteocephalusEcologyPhylogenetic treeosteocephalus010607 zoologyBiodiversityGeneral. Including nature conservation geographical distributionZoologyQH1-199.5Biologymolecular toolsbiology.organism_classification010603 evolutionary biology01 natural sciencesHylidaeSpecies groupQH540-549.5Ecology Evolution Behavior and SystematicsbiodiversityAmazon basinNeotropical Biodiversity
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Can differences in microbial abundances help explain enhanced N2O emissions in a permanent grassland under elevated atmospheric CO2?

2011

nirSGlobal and Planetary ChangegeographyN2O emissionsDenitrificationgeography.geographical_feature_categorydenitrificationEcologyEcology[SDE.MCG]Environmental Sciences/Global ChangesGrasslandAOAAOBsoilEnrichissement en gaz carboniqueConcentration élevée en CO2nosZFACEammonia oxidationEnvironmental ChemistryEnvironmental sciencenirKGeneral Environmental Science
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Noise Reduction and Gap Filling of fAPAR Time Series Using an Adapted Local Regression Filter

2014

Time series of remotely sensed data are an important source of information for understanding land cover dynamics. In particular, the fraction of absorbed photosynthetic active radiation (fAPAR) is a key variable in the assessment of vegetation primary production over time. However, the fAPAR series derived from polar orbit satellites are not continuous and consistent in space and time. Filtering methods are thus required to fill in gaps and produce high-quality time series. This study proposes an adapted (iteratively reweighted) local regression filter (LOESS) and performs a benchmarking intercomparison with four popular and generally applicable smoothing methods: Double Logistic (DLOG), sm…

noise010504 meteorology & atmospheric sciencesRemote sensing applicationComputer scienceNoise reduction0211 other engineering and technologies02 engineering and technologyLand cover01 natural sciencesfAPAR; noise; MODIS; time series; filtering; interpolation; LOESSSmoothing splineLoessLOESSlcsh:Science021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingLocal regressionFilter (signal processing)Vegetation15. Life on landfilteringSnowinterpolationNoiseMODISfAPARGeneral Earth and Planetary Scienceslcsh:Qtime seriesSmoothingInterpolationRemote Sensing
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Aliens and dragons: purposefully-framed play and non-standard learning methods in teaching evolutionary processes to primary school pupils

2023

Evolutionary processes lie at the base of the entire observable biodiversity, both at present and in the geological past (i.e., in the fossil record). For this reason, the teaching of evolution should receive more recognition than it currently has (e.g., in Poland) and become accurately applied from the early formal education stages onwards. To test the possibility of effective teaching of evolution to primary school pupils, workshops using non-standard learning methods (‘purposefully-framed play’) were organised during childrens’ university (UNIKIDS) courses of one-hour sessions for 33 groups, comprising several to 20 participants, aged 7 to 12. The final task for all participants was to p…

non-formal educationpalaeontological educationGeneral Earth and Planetary Sciencesbiological educationgeoeducationGeologos
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Diurnal Cycle Relationships between Passive Fluorescence, PRI and NPQ of Vegetation in a Controlled Stress Experiment

2017

In order to estimate vegetation photosynthesis from remote sensing observations; some critical parameters need to be quantified. From all absorbed light; the plant needs to release any excess that is not used for photosynthesis; by non-photochemical quenching; by fluorescence emission and unregulated thermal dissipation. Non-photochemical quenching (NPQ) processes are controlled photoprotective mechanisms which; once activated; strongly control the dynamics of photochemical efficiency. With illumination conditions increasing and decreasing during a diurnal cycle; photoprotection mechanisms needs to change accordingly. The goal of this work is to quantify dynamic NPQ; measured from active fl…

non-photochemical energy dissipation0106 biological sciencesPhotoinhibition010504 meteorology & atmospheric sciencesSciencedroughtsolar-induced fluorescence (SIF)PhotosynthesisPhotochemical Reflectance IndexAtmospheric sciencesFLuorescence EXplorer01 natural sciencesstressDiurnal cycle0105 earth and related environmental sciencesRemote sensingphotosynthesisQuenching (fluorescence)Chemistry(FLEX)Qdrought; stress; non-photochemical energy dissipation; solar-induced fluorescence (SIF); photosynthesis; non-photochemical quenching (NPQ); Photochemical Reflectance Index (PRI); FLuorescence EXplorer; (FLEX)15. Life on landFluorescencePhotochemical Reflectance Index (PRI)non-photochemical quenching (NPQ)Photosynthetically active radiationPhotoprotectionGeneral Earth and Planetary Sciences010606 plant biology & botanyRemote Sensing; Volume 9; Issue 8; Pages: 770
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Decay assessment of stone-built cultural heritage: The case study of the cosenza cathedral façade (south calabria, italy)

2021

This study aims to assess the different decay phenomena affecting the Cosenza Cathedral façade (Calabria, South Italy) through the evaluation of the relative damage indices. For this goal, a multidisciplinary approach was applied exploiting both nondestructive and microdestructive techniques. Such a combination enabled proposing an intervention priority scale that can be helpful to institutions when planning a prompt restoration intervention. The results suggest the efficiency of this approach to obtain a multidisciplinary diagnostic and conservation system for the management and valorization of the Cultural Heritage also in terms of monitoring, maintenance, and selection of the most suitab…

nondestructive techniques; microdestructive techniques; stone deterioration; damage indices; Cosenza; ItalyScienceQCosenza Damage indices Italy Microdestructive techniques Nondestructive techniques Stone deteriorationmicrodestructive techniquesnondestructive techniquesCosenzaCultural heritageStone deteriorationGeographydamage indicesMicrodestructive techniqueItalyNondestructive techniqueMultidisciplinary approachDamage indiceGeneral Earth and Planetary SciencesFacadeEnvironmental planningSettore GEO/09 -Georis. Miner.e Appl.Mineral.-Petrogr. per l'Ambi.ed i B.Cult.
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DERECHO A UNA CULTURA DE PAZ. EL CAMINO DESDE LA EDUCACIÓN.

2016

La cultura de paz, de acuerdo con la comunidad internacional, implica la adhesión a los principios de libertad, justicia, democracia, tolerancia, solidaridad, cooperación, pluralismo, diversidad cultural, diálogo y entendimiento a todos los niveles de la sociedad y entre las naciones; y animados por un entorno nacional e internacional que favorezca la paz. En esta línea, la UNESCO declaró el periodo comprendido entre 2001 y 2010 como el Decenio Internacional para una Cultura de Paz y no violencia para los niños del mundo. En este contexto, la llamada Educación para una Cultura de Paz (ECP) pretende contribuir a la construcción de un nuevo orden internacional basado en un concepto de paz pos…

noviolenciapazGeneral Earth and Planetary Sciencescultura de pazeducaciónGeneral Environmental ScienceRevista ORG & DEMO
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Spectra of high-mass X-ray binaries

2016

High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by the accretion of matter from the massive companion onto a neutron star. The accreting material comes from either the strong stellar wind in binaries with supergiant companions or the circumstellar disk in Be/X-ray binaries. In either case, the H{alpha} line stands out as the main source of information about the state of the accreting material. We present the results of our monitoring program to study the long-term variability of the H{alpha} line in high-mass X-ray binaries. Our aim is to characterise the optical variability timescales and study the interaction between the neutron star and the accreting…

observational astronomyAstrophysics and AstronomyStellar AstronomyX-ray binary starsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsX ray binary starsNatural SciencesAstrophysics::Galaxy AstrophysicsSpectroscopy
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