Search results for " format"

showing 10 items of 2156 documents

A spatial analysis of new business formation: Replicative vs innovative behaviour

2017

Abstract Using spatial econometric tools, the paper examines the spatial structure of new business formation of Italian regions during the period 2004–2007. In particular, the study empirically investigates whether new business formation in a given geographical area may be explained in terms of replicative and/or innovative entrepreneurial behaviour in each area as well as in the neighbouring areas. Additionally, the analysis focuses on the influence of urbanization on the birth of new firms. From the estimation of a Spatial Durbin Model, we find a significant degree of spatial dependence among Italian regions not only in new business formation but also in some of its determinants. We also …

Statistics and ProbabilityEstimationSpatial structureUrbanization05 social sciencesSpatial analysis0211 other engineering and technologies021107 urban & regional planning02 engineering and technologyManagement Monitoring Policy and LawDegree (music)Replicative and innovative behaviourUrbanizationSettore SECS-S/03 - Statistica Economica0502 economics and businessEconomicsEconomic geography050207 economicsComputers in Earth SciencesSpatial dependenceNew business formationSpatial Statistics
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From deterministic cellular automata to coupled map lattices

2016

A general mathematical method is presented for the systematic construction of coupled map lattices (CMLs) out of deterministic cellular automata (CAs). The entire CA rule space is addressed by means of a universal map for CAs that we have recently derived and that is not dependent on any freely adjustable parameters. The CMLs thus constructed are termed real-valued deterministic cellular automata (RDCA) and encompass all deterministic CAs in rule space in the asymptotic limit $\kappa \to 0$ of a continuous parameter $\kappa$. Thus, RDCAs generalize CAs in such a way that they constitute CMLs when $\kappa$ is finite and nonvanishing. In the limit $\kappa \to \infty$ all RDCAs are shown to ex…

Statistics and ProbabilityGeneral Physics and AstronomyFOS: Physical sciencesPattern Formation and Solitons (nlin.PS)Space (mathematics)01 natural sciences010305 fluids & plasmasLinear stability analysis0103 physical sciencesLimit (mathematics)Statistical physics010306 general physicsMathematical PhysicsBifurcationPhysicsCellular Automata and Lattice Gases (nlin.CG)Quiescent stateStatistical and Nonlinear PhysicsNonlinear Sciences - Chaotic DynamicsNonlinear Sciences - Pattern Formation and SolitonsCellular automatonNonlinear Sciences - Adaptation and Self-Organizing SystemsHomogeneousModeling and SimulationContinuous parameterChaotic Dynamics (nlin.CD)Adaptation and Self-Organizing Systems (nlin.AO)Nonlinear Sciences - Cellular Automata and Lattice Gases
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IndElec: A Software for Analyzing Party Systems and Electoral Systems

2011

IndElec is a software addressed to compute a wide range of indices from electoral data, which are intended to analyze both party systems and electoral systems in political studies. Further, IndElec can calculate such indices from electoral data at several levels of aggregation, even when the acronyms of some political parties change across districts. As the amount of information provided by IndElec may be considerable, this software also aids the user in the analysis of electoral data through three capabilities. First, IndElec automatically elaborates preliminary descriptive statistical reports of computed indices. Second, IndElec saves the computed information into text files in data matri…

Statistics and ProbabilityWeb browserDatabaseComputer sciencebusiness.industrydisproportionalityparty systemcomputer.software_genreFile formatVisualizationRange (mathematics)Softwareelectoral systemStatistics Probability and Uncertaintybusinessparty dimensionscomputerlcsh:Statisticslcsh:HA1-4737SoftwareWord (computer architecture)Statistical softwareGraphical user interfaceJournal of Statistical Software
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Dynamics of Pattern Formation in Biomimetic Systems

2008

This paper is an attempt to conceptualize pattern formation in self-organizing systems and, in particular, to understand how structures, oscillations or waves arise in a steady and homogenous environment, a phenomenon called symmetry breaking. The route followed to develop these ideas was to couple chemical oscillations produced by Belousov-Zhabotinsky reaction with confined reaction environments, the latter being an essential requirement for any process of Life. Special focus was placed on systems showing organic or lipidic compartments, which represent more reliable biomimetic matrices.

Statistics and Probability{CHEMICAL} {OSCILLATORS}Belousov-Zhabotinsky reactionLipid BilayersPattern formationNanotechnology{CHEMICAL} {OSCILLATORS}; Lipid systems; Reverse microemulsionsModels BiologicalTuring structuresGeneral Biochemistry Genetics and Molecular BiologyDiffusionBiomimeticsChemical oscillatorsAnimalsSymmetry breakingPhysicsGeneral Immunology and MicrobiologyChemistry PhysicalSystems BiologyApplied MathematicsLipid systemsBiomimetic systemsGeneral MedicineBelousov-Zhabotinsky reaction; Chemical oscillators; Turing structures; Biomimetic systems; Lipid systems; Reverse microemulsionsReverse microemulsionsBelousov–Zhabotinsky reactionModeling and SimulationEmulsionsGeneral Agricultural and Biological SciencesBiological system
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Mapping accretion and its variability in the young open cluster NGC 2264: A study based on u-band photometry

2014

We aim at characterizing the accretion properties of several hundred members of the star-forming cluster NGC 2264 (3 Myr). We performed a deep u,g,r,i mapping and a simultaneous u+r monitoring of the region with CFHT/MegaCam in order to directly probe the accretion process from UV excess measurements. Photometric properties and stellar parameters are determined homogeneously for about 750 monitored young objects, spanning the mass range 0.1-2 Mo. About 40% are classical (accreting) T Tauri stars, based on various diagnostics (H_alpha, UV and IR excesses). The remaining non-accreting members define the (photospheric+chromospheric) reference UV emission level over which flux excess is detecte…

Stellar massAstrophysics::High Energy Astrophysical PhenomenaStars: formationPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPhotometry (optics)Accretion rateAccretion accretion diskStars: low-maAstrophysics::Solar and Stellar AstrophysicseducationAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physicseducation.field_of_studyDetection thresholdAstronomy and AstrophysicsAstronomy and AstrophysicUltraviolet: starAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar Astrophysicsindividual: NGC 2264; Stars: formation; Stars: low-mass; Stars: pre-main sequence; Ultraviolet: stars; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Open clusters and associations]Space and Planetary ScienceOpen clusters and associations: individual: NGC 2264Stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen cluster
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Gaia DR2 reveals a star formation burst in the disc 2-3 Gyr ago

2019

We use Gaia DR2 magnitudes, colours and parallaxes for stars with G<12 to explore a 15-dimensional space that includes simultaneously the initial mass function (IMF) and a non-parametric star formation history (SFH) for the Galactic disc. This inference is performed by combining the Besancon Galaxy Model fast approximate simulations (BGM FASt) and an approximate Bayesian computation algorithm. We find in Gaia DR2 data an imprint of a star formation burst 2-3 Gyr ago, in the Galactic thin disc domain, and a present star formation rate (SFR) of about 1 Msun. Our results show a decreasing trend of the SFR from 9-10 Gyr to 6-7 Gyr ago. This is consistent with the cosmological star formation …

Stellar massFOS: Physical sciencesPerturbation (astronomy)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsmass function -galaxiesstar formation rate01 natural sciencesdisk -Galaxy0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicsluminosity functionDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsstellar content -Hertzsprung-Russell and C-M diagramsstars010308 nuclear & particles physicsStar formationDiscos (Astrofísica)Astronomy and Astrophysicsstellar initial mass functioninteractionsGalaxiesAstrophysics - Astrophysics of GalaxiesStarsGalaxyRedshiftevolution -Galaxystar formation historyGalàxiesEstelsStarsGalaxyGalaxies evolutionDisks (Astrophysics)[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)galaxy mergeEvolució de les galàxiesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs

2015

Aims: Long gamma-ray bursts (LGRBs) are associated with massive stars and are therefore linked to star formation. However, the conditions needed for the progenitor stars to produce LGRBs can affect the relation between the LGRB rate and star formation. By using the power of a complete LGRB sample, our long-term aim is to understand whether such a bias exists and, if it does, what its origin is. Methods: To reach our goal we use the Swift/BAT6 complete sample of LGRBs. In this first paper, we build the spectral energy distribution (SED) of the 14 z ⋆) from SED fitting. To investigate the presence of a bias in the LGRB-star formation relation we compare the stellar mass distribution of the LG…

Stellar massMetallicityAstrophysics::High Energy Astrophysical PhenomenaPopulationgamma-ray burst: generalAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsQCAstrophysics::Galaxy AstrophysicsQBPhysicseducation.field_of_study010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsGalaxyStarsgalaxies: photometrySpace and Planetary Sciencegalaxies: star formationSpectral energy distributionAstrophysics::Earth and Planetary AstrophysicsGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Lyman break and ultraviolet-selected galaxies at z ~ 1 - II. PACS 100μm/160μm FIR detections

2013

In this work, we report the Photodetector Array Camera and Spectrometer (PACS) 100 μm/160 μm detections of a sample of 42 GALEX-selected and far-infrared (FIR)-detected Lyman break galaxies (LBGs) at z ~ 1 located in the Cosmic Evolution Survey (COSMOS) field and analyse their ultraviolet (UV) to FIR properties. The detection of these LBGs in the FIR indicates that they have a dust content high enough so that its emission can be directly detected. According to a spectral energy distribution (SED) fitting with stellar population templates to their UV-to-near-IR observed photometry, PACS-detected LBGs tend to be bigger (Reff ~ 4.1 kpc), more massive [log (M*/M⊙) ~ 10.7], dustier [Es(B - V) ~ …

Stellar populationAstrophysicsgalaxies [Radio continuum]medicine.disease_causestar formation [Galaxies]Physical cosmologyhigh-redshift [Galaxies]galaxies [Infrared]galaxies: high-redshiftmedicineLuminous infrared galaxyPhysicsStar formationinfrared: galaxieAstronomyAstronomy and Astrophysicsevolution [Galaxies]RedshiftGalaxygalaxies [Ultraviolet]Space and Planetary Sciencegalaxies: star formationultraviolet: galaxiesSpectral energy distributionradio continuum: galaxiegalaxies: evolutionUltraviolet
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CGCG 480-022: A Distant Lonesome Merger?

2006

[EN]We present a complete analysis, which includes morphology, kinematics, stellar populations, and N-body simulations, of CGCG 480-022, the most distant (cz = 14,317 km s-1) isolated galaxy studied so far in such detail. The results all support the hypothesis that this galaxy has suffered a major merger event with a companion of ~0.1 times its mass. Morphology reveals the presence of a circumnuclear ring and possibly further ring debris. The radial velocity curve looks symmetrical, while the velocity dispersion increases with radius, reaching values that do not correspond to a virialized system. Moreover, this galaxy deviates significantly from the fundamental plane and the Faber-Jackson r…

Stellar populationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematicsAstrophysicsabundances [galaxies]kinematics and dynamics [galaxies]galaxies: interactionsgalaxies: kinematics and dynamicsAstrophysics::Galaxy AstrophysicsPhysicsgalaxies: individual (CGCG 480 022)interactions [galaxies]Instituto de Ciencias del PatrimonioStar formationAstrophysics (astro-ph)Velocity dispersionAstronomy and Astrophysicsindividual (CGCG 480 022) [galaxies]GalaxyInstitute of Heritage SciencesRadial velocitySpace and Planetary ScienceIncipitstructure [galaxies]galaxies: structuregalaxies: abundancesAstrophysics::Earth and Planetary AstrophysicsFundamental plane (elliptical galaxies)n-body simulations [methods]methods: n-body simulationsThe Astrophysical Journal
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The ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies atz< 0.3

2017

Reproduced with permission from Astronomy & Astrophysics

Stellar populationMetallicityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicselliptical and lenticular cD [Galaxies]01 natural sciencescDPhotometry (optics)0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgalaxies: formationgalaxies: elliptical and lenticularSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]Physics010308 nuclear & particles physicsphotometry [Galaxies]FísicaAstronomy and Astrophysicsevolution [Galaxies]Astrophysics - Astrophysics of Galaxiesformation [Galaxies]Galaxy2d analysisEarly typeGalaxies: elliptical and lenticular cDgalaxies: photometrySpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary Astrophysicsgalaxies: evolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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