Search results for "GAL"

showing 10 items of 9260 documents

The close classical T Tauri binary V4046 Sgr: Complex magnetic fields & distributed mass accretion

2011

We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes within the close binary system V4046 Sgr, hosting two partly-convective classical T Tauri stars of masses ~0.9 Msun and age ~12 Myr. In this paper, we present time-resolved spectropolarimetric observations collected in 2009 September with ESPaDOnS at the Canada-France-Hawaii Telescope (CFHT) and covering a full span of 7d or ~2.5 orbital/rotational cycles of V4046 Sgr. Small circularly polarised Zeeman signatures are detected in the photospheric absorption lines but not in the accretion-powered emission lines of V4046 Sgr, thereby demonstrating that both system components host lar…

stars: formation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]stars: individual: V4046 SgrAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsstars: imagingtechniques: polarimetricSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar Astrophysicsstars: rotation[SDU]Sciences of the Universe [physics]stars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysicstechniques: polarimetric stars: formation stars: imaging stars: individual: V4046 Sgr stars: magnetic fields stars: rotationAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics
researchProduct

Evidence of a non-conservative mass transfer in the ultra-compact X-ray source XB 1916-053

2020

The dipping source XB 1916-053 is a compact binary system with an orbital period of 50 min harboring a neutron star. Using ten new {\it Chandra} observations and one {\it Swift/XRT} observation, we are able to extend the baseline of the orbital ephemeris; this allows us to exclude some models that explain the dip arrival times. The Chandra observations provide a good plasma diagnostic of the ionized absorber and allow us to determine whether it is placed at the outer rim of the accretion disk or closer to the compact object. From the available observations we are able to obtain three new dip arrival times extending the baseline of the orbital ephemeris from 37 to 40 years. From the analysis…

stars: individual: XB 1916-053Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesaccretion0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsaccretion disksApsidal precessionAstronomy and AstrophysicsMass ratioOrbital periodRedshiftNeutron starSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Gravitational redshiftAstronomy & Astrophysics
researchProduct

ARGUMENTS FOR THE ESTABLISHMENT OF A SOVEREIGN INVESTMENT FUND IN ROMANIA

2013

The creation of the national development fund was approved in 2006 through the specific legislation. The main argument in supporting the idea of creating this fund was the fact that Romania still had to privatize some more governmental ownership companies and the sums that would be obtained were going to be used according to some very precise rules. Another argument was that the executive power had to assure the financing of some major infrastructure investment projects, to assure the local contribution of the project financed by structural funds and to assure de necessary funds for solving the problems caused by the retrocession of some buildings. The audit report of the Romanian Court of …

state assets privatization legal regularity inter-ministerial bodyStudies in Business and Economics
researchProduct

The ALHAMBRA survey: evolution of galaxy clustering since z∼1

2014

We study the clustering of galaxies as function of luminosity and redshift in the range $0.35 < z < 1.25$ using data from the Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) survey. The ALHAMBRA data used in this work cover $2.38 \mathrm{deg}^2$ in 7 independent fields, after applying a detailed angular selection mask, with accurate photometric redshifts, $��_z \lesssim 0.014 (1+z)$, down to $I_{\rm AB} < 24$. Given the depth of the survey, we select samples in $B$-band luminosity down to $L^{\rm th} \simeq 0.16 L^{*}$ at $z = 0.9$. We measure the real-space clustering using the projected correlation function, accounting for photometric redshifts uncert…

statistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCorrelation function (astronomy)01 natural sciencesPhysical cosmologyLuminosityLarge-scale structure of Universe.0103 physical sciencesRange (statistics)distances and redshifts [Galaxies]Sample variance10. No inequalitydata analysis [Methods]observations [Cosmology]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsGalaxyRedshiftSpace and Planetary ScienceHaloAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

THE ALHAMBRA SURVEY: EVOLUTION OF GALAXY SPECTRAL SEGREGATION

2016

arXiv:1601.03668v1

statistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of universeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMethods statisticalGalaxies: distances and redshiftsMethods: data analysis0103 physical sciencesdistances and redshifts [Galaxies]observations [Cosmology]data analysis [Methods]010303 astronomy & astrophysicsMethods: statisticalAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsCosmology: observationsFísicaAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography

2021

Ilbert, O., et al. (Euclid Collaboration)

statistical [Methods]IMPACTUNIVERSEAstrophysics01 natural sciencesDark energyGalaxies: distances and redshiftdark energyPHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingPhotometric redshiftmedia_commonPhysicsdistances and redshift [Galaxies]Dark energy; Galaxies: distances and redshifts; Methods: statisticalSIMULATIONastro-ph.CO3103 Astronomy and AstrophysicsProbability distributionSpectral energy distributiongalaxies: distances and redshiftsAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)530 Physicsastro-ph.GAmedia_common.quotation_subjectFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics1912 Space and Planetary Science0103 physical sciencesdistances and redshifts [Galaxies]/dk/atira/pure/subjectarea/asjc/1900/1912DISTRIBUTIONSmethods: statistical010308 nuclear & particles physicsAstronomy and AstrophysicsPERFORMANCE115 Astronomy Space scienceAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyUniverseRedshiftSTELLARRESOLUTIONSpace and Planetary Science10231 Institute for Computational ScienceAstrophysics of Galaxies (astro-ph.GA)Dark energy/dk/atira/pure/subjectarea/asjc/3100/3103[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Measuring galaxy segregation with the mark connection function

2010

(abridged) The clustering properties of galaxies belonging to different luminosity ranges or having different morphological types are different. These characteristics or `marks' permit to understand the galaxy catalogs that carry all this information as realizations of marked point processes. Many attempts have been presented to quantify the dependence of the clustering of galaxies on their inner properties. The present paper summarizes methods on spatial marked statistics used in cosmology to disentangle luminosity, colour or morphological segregation and introduces a new one in this context, the mark connection function. The methods used here are the partial correlation functions, includi…

statistical [Methods]Spatial correlationCosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of UniversePopulationFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCorrelation function (astronomy)UNESCO::ASTRONOMÍA Y ASTROFÍSICAUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasdata analysis [Methods]educationCluster analysisPartial correlationPhysicseducation.field_of_studyAstronomy and AstrophysicsFunction (mathematics)GalaxyLarge-scale structure of Universe; Methods : data analysis; Methods : statisticalSpace and Planetary Science:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

A photometric study of Be stars located in the seismology fields of COROT

2007

Context: In preparation for the COROT mission, an exhaustive photometric study of Be stars located in the seismology fields of the COROT mission has been performed. The very precise and long-time-spanned photometric observations gathered by the COROT satellite will give important clues of the origin of the Be phenomenon. Aims: The aim of this work is to find short-period variable Be stars located in the seismology fields of COROT and to study and characterise their pulsational properties. Methods: Light curves obtained at the Observatorio de Sierra Nevada together with data from Hipparcos and ASAS-3 of a total of 84 Be stars have been analysed in order to search for short-term variations. W…

statistics [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Otras [UNESCO]FOS: Physical sciencesoscillations (including pulsations) [Stars]Context (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences0103 physical sciencesUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::OtrasAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsphotometric [Techniques]Astrophysics (astro-ph)Astronomy and AstrophysicsLight curveStars : emission-line Be; Stars : oscillations (including pulsations); Stars : statistics; Techniques : photometricStarsemission-line Be [Stars]Space and Planetary ScienceSatelliteAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSeismology:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
researchProduct

Stato di emergenza e legalità costituzionale alla prova della pandemia

2022

The need to outline a satisfactory relationship between emergency and constitutional legality has accompanied the evolution of public law, posing questions that are not fully resolved. The debate on the issue is back in vogue with the pandemic emergency, in relation to the issues related to containment measures. The paper traces the related matter, also in light of the interpretation offered by the judgments that the Constitutional Court has pronounced, in particular in relation to the territorial balance of emergency powers and the system of sources of law.

stato di eccezione stato di emergenza legalità costituzionale diritti fondamentali fonti del dirittoSettore IUS/08 - Diritto Costituzionale
researchProduct

Stimula kontrasta un virziena ietekme uz sakādisko acu kustību parametriem

2022

Darbs ir uzrakstīts latviešu valodā uz 41 lapaspusēm. Tas satur 25 attēlus, 2 tabulas, 3 pielikumus un 46 atsauces uz literatūras avotiem. Darba mērķis ir novērtēt stimula kontrasta un virziena ietekmi uz sakāžu parametriem (sakādisko acu kustību latences, precizitātes un maksimālā ātruma rādītājiem). Pētījumā piedalījās 15 dalībnieki (no 21 līdz 29 gadiem). Acu kustibas tika pierakstītas ar Tobii Pro Fusion acu kustību pieraksta iekārtu (250Hz). Sakādisko acu kustību stimuli ar dažādiem kontrasta līmeņiem tika demonstrēti uz četriem dažādiem foniem četros dažādos virzienos. Rezultāti norāda būtisku stimula virziena ietekmi uz latenci un maksimālo ātrumu pelēkā fonā 30 cd/m2 (negatīva un po…

stimula parametrisakādiskās acu kustībassakādisko acu kustību parametrisakādisko acu kustību galvenā sakarībaFizikapsihofizikālā metode
researchProduct