Search results for "Planetary Science"

showing 10 items of 4367 documents

The ALHAMBRA survey: reliable morphological catalogue of 22 051 early- and late-type galaxies

2013

Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) is photometric survey designed to trace the cosmic evolution and cosmic variance. It covers a large area of ~4 deg2 in eight fields, where seven fields overlap with other surveys, allowing us to have complementary data in other wavelengths. All observations were carried out in 20 continuous, medium band (30 nm width) optical and 3 near-infrared (JHK) bands, providing the precise measurements of photometric redshifts. In addition, morphological classification of galaxies is crucial for any kind of galaxy formation and cosmic evolution studies, providing the information about star formation histories, their environme…

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Galaxies: statisticsFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsEuropean Social FundSurveys01 natural sciencesstatistics [Galaxies]0103 physical sciences10. No inequality010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsLate typeAstronomyAstronomy and AstrophysicsSpace and Planetary ScienceResearch councilfundamental parameters [Galaxies]Christian ministry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Data releaseAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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The ALHAMBRA survey: An empirical estimation of the cosmic variance for merger fraction studies based on close pairs

2014

[Aims]: Our goal is to estimate empirically the cosmic variance that affects merger fraction studies based on close pairs for the first time. [Methods]: We compute the merger fraction from photometric redshift close pairs with 10 h−1 kpc ≤ rp ≤ 50 h−1 kpc and Δv ≤ 500 km s−1 and measure it in the 48 sub-fields of the ALHAMBRA survey. We study the distribution of the measured merger fractions that follow a log-normal function and estimate the cosmic variance σv as the intrinsic dispersion of the observed distribution. We develop a maximum likelihood estimator to measure a reliable σv and avoid the dispersion due to the observational errors (including the Poisson shot noise term). [Results]: …

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Stellar massGalaxies: statisticsFOS: Physical sciencesAstrophysicsinteractions [Galaxies]Astrophysics::Cosmology and Extragalactic AstrophysicsPoisson distribution01 natural sciencesLuminositysymbols.namesakestatistics [Galaxies]0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysics[PHYS]Physics [physics]COSMIC cancer database010308 nuclear & particles physicsAstronomy and AstrophysicsCosmic varianceRedshiftGalaxyGalaxies: interactionsSpace and Planetary Sciencefundamental parameters [Galaxies]symbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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SHARDS: A global view of the star formation activity at z~0.84 and z~1.23

2015

et al.

Galaxies: generalAstrofísicaStellar massFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]Luminosityhigh-redshift [Galaxies]emission lines [Quasars]Stellar evolutionAstrophysics::Galaxy AstrophysicsCosmic dustPhysicsQuasars: emission linesGalaxies: star formationStar formationphotometry [Galaxies]Galaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsQuasarGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesRedshiftGalaxyAstronomíaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)
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Evolution of Balmer jump selected galaxies in the ALHAMBRA survey

2016

Extragalactic astronomy.-- et al.

Galaxies: generalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesevolution [Galaxy]high-redshift [Galaxies]Galactic haloBalmer jump0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicshalo [Galaxy]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]PhysicsGalaxy: evolution010308 nuclear & particles physicsphotometry [Galaxies]Astrophysics::Instrumentation and Methods for AstrophysicsGalaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyPhysics::History of PhysicsGalaxy: haloSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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The ALHAMBRA survey: accurate merger fractions derived by PDF analysis of photometrically close pairs

2015

[Aims]: Our goal is to develop and test a novel methodology to compute accurate close-pair fractions with photometric redshifts. [Methods]: We improved the currently used methodologies to estimate the merger fraction fm from photometric redshifts by (i) using the full probability distribution functions (PDFs) of the sources in redshift space; (ii) including the variation in the luminosity of the sources with z in both the sample selection and the luminosity ratio constrain; and (iii) splitting individual PDFs into red and blue spectral templates to reliably work with colour selections.We tested the performance of our new methodology with the PDFs provided by the ALHAMBRA photometric survey.…

Galaxies: statisticsmedia_common.quotation_subjectAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsEuropean Social Fundinteractions [Galaxies]Public administration01 natural sciencesstatistics [Galaxies]Excellence0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSmedia_commonPhysics[PHYS]Physics [physics]Government010308 nuclear & particles physicsGalaxies: evolutionAstronomy and Astrophysicsevolution [Galaxies]Galaxies: interactionsWork (electrical)Space and Planetary ScienceResearch council[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation

2023

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cover the wide range of wavelengths where atmospheric absorption and emission limit the use of ground facilities. Thanks to continuing technological improvements, miniaturised space instruments operating as distributed-aperture constellations are offering new capabilities for the study of high energy transients to complement ageing existing satellites. In this paper we characterise the performance of the upcoming joint SpIRIT + HERMES-TP/SP nano-satellite constellation for the localisation of high-energy transients th…

Gamma ray transient sourceHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceX-ray transient sourceSpace telescopeTime domain astronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

2007

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the the…

Gamma rays: burstsNormalization (statistics)PhysicsRange (particle radiation)MuonAstrophysics::High Energy Astrophysical PhenomenaGamma rays: bursts; Neutrinos; TelescopesAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoincidenceSpace and Planetary ScienceCascadeAstronomiaDiffuse fluxHigh Energy Physics::ExperimentNeutrinosNeutrinoGamma-ray burstTelescopesThe Astrophysical Journal
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García-Izquierdo, A. L. (Editor). (2017). Ergonomía y psicosociología aplicada a la prevención de riesgos laborales

2019

García-Izquierdo A. L. (Editor). (2017). Ergonomía y psicosociología aplicada a la prevención de riesgos laborales Artículo:PSICOLOGÍA [UNESCO]General Earth and Planetary SciencesUNESCO::PSICOLOGÍAGeneral Environmental Science
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Periodic volcanic degassing behavior: The Mount Etna example

2013

[1] In contrast to the seismic and infrasonic energy released from quiescent and erupting volcanoes, which have long been known to manifest episodes of highly periodic behavior, the spectral properties of volcanic gas flux time series remain poorly constrained, due to a previous lack of hightemporal resolution gas-sensing techniques. Here we report on SO2 flux measurements, performed on Mount Etna with a novel UV imaging technique of unprecedented sampling frequency (0.5Hz), which reveal, for the first time, a rapid periodic structure in degassing from this target. These gas flux modulations have considerable temporal variability in their characteristics and involve two period bands: 40–250…

Gas bubble010504 meteorology & atmospheric sciencesPeriod (periodic table)Mount Etna; periodic gas flux; UV camera; volcanic tremor; Geophysics; Earth and Planetary Sciences (all)InfrasoundFluxUV camera010502 geochemistry & geophysics01 natural sciences0105 earth and related environmental sciencesgeographygeography.geographical_feature_categorySpectral propertiesGeophysicsvolcanic tremorMountMount Etna; periodic gas flux; UV camera; volcanic tremor; Earth and Planetary Sciences (all); GeophysicsGeophysicsVolcano13. Climate actionGeneral Earth and Planetary SciencesMount EtnaImaging techniqueperiodic gas fluxMount Etna; periodic gas flux; UV camera; volcanic tremorEarth and Planetary Sciences (all)GeologySeismology
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Wage Gap as a Possible Determinant of Gender Inequality

2021

Recent academic researchers have indicated that there are possible inequalities concerning work and pay in different countries, professions and economic sectors. The aim of current research is to analyse recent scientific findings on the wage gap depending on gender and empirical data in Latvia using EU-SILC surveys, Labour Surveys and monthly statistical data on wages and salaries for women and men. The findings indicated that in various economic fields and occupations women were under-represented, and amongst most of these fields the modal net wage interval for women was lower than the modal net wage interval for men. It was also concluded that in January 2018 the average gross income fro…

Gender inequalityGlass ceilingEmpirical datainequalityInequalityWages and salariesEconomic sectormedia_common.quotation_subjectWageGross incomeEconomicsGeneral Earth and Planetary Sciences:SOCIAL SCIENCES::Business and economics [Research Subject Categories]Demographic economicswage gapglass ceilinghealth care economics and organizationsGeneral Environmental Sciencemedia_common
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