Search results for "Spectroscopy"

showing 10 items of 10293 documents

Abundance signature of M dwarf stars

2020

Most of our current knowledge on planet formation is still based on the analysis of main-sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M-dwarf planet hosts are still missing. We aim to test whether the correlations between the metallicity, individual chemical abundances, and mass of the star and the presence of different type of planets found for FGK stars still holds for the less massive M dwarf stars. Methods to determine in a consistent way stellar abundances of M dwarfs from high-resolution optical spectra are still missing. The present work is a first attempt to fill this gap. We analyse in a coherent and homogeneous way a large sample of M dwarf…

Astrophysics and AstronomyRadial velocityPhysicsExoplanetsChemical abundancesexoplanet astronomyAstrophysics::Cosmology and Extragalactic AstrophysicsLate type starsstellar astronomyInterdisciplinary Astronomyobservational astronomyM starsMetallicityAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesLate-type starsAstrophysics::Galaxy AstrophysicsSpectroscopy
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Radio observations of the HDFS region. IV.

2011

The Australia Telescope Hubble Deep Field-South (ATHDF-S) survey of the Hubble Deep Field-South (HDF-S) reaches sensitivities of ~10uJy at 1.4, 2.5, 5.2, and 8.7GHz, making the ATHDF-S one of the deepest surveys ever performed with the Australia Telescope Compact Array (ATCA). Here, we present the optical identifications of the ATHDF-S radio sources using data from the literature. We find that ~66% of the radio sources have optical counterparts to I=23.5mag. Deep Hubble Space Telescope (HST) imaging of the area identifies a further 12% of radio sources. We present new spectroscopic observations for 98 of the radio sources and supplement these spectroscopic redshifts with photometric ones ca…

Astrophysics and AstronomyRadio sourcesAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRedshiftedSurveysCosmologyOptical astronomyobservational astronomyPhotometryAstrophysics::Solar and Stellar AstrophysicsWide-band photometryRadio astronomyNatural SciencesAstrophysics::Galaxy AstrophysicsInfrared photometrySpectroscopyWide band photometry
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Monte Carlo simulation of the response of ESR dosimeters added with gadolinium exposed to thermal, epithermal and fast neutrons

2009

Abstract Monte Carlo numerical calculations of the response of alanine and ammonium tartrate ESR (electron spin resonance) dosimeters exposed to neutron fields with different energy spectra are reported. Results have been obtained for various gadolinium concentrations inside the dosimeters. Furthermore, in order to simulate the in-phantom response we have carried out calculations by varying the depth of the dosimeter. We have found that a large enhancement is obtained for thermal neutrons, because of the very high capture cross section of gadolinium to thermal neutrons. A good enhancement was obtained for epithermal neutrons, whereas the sensitivity improvement in the case of fast neutron i…

Astrophysics::High Energy Astrophysical PhenomenaGadoliniumPhysics::Medical PhysicsMonte Carlo methodchemistry.chemical_elementGadoliniumSpectral lineFast NeutronsHumansDosimetryNeutronRadiometryNuclear ExperimentTartratesAlanineRadiationDosimeterPhantoms ImagingRadiotherapy Planning Computer-AssistedESR dosimetry gadolinium neutronsRadiochemistryElectron Spin Resonance SpectroscopyNeutron Capture TherapyNeutron temperatureNeutron capturechemistryAtomic physicsMonte Carlo MethodApplied Radiation and Isotopes
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The novel HALO mini-DOAS instrument: inferring trace gas concentrations from airborne UV/visible limb spectroscopy under all skies using the scaling …

2017

Abstract. We report on a novel six-channel optical spectrometer (further on called mini-DOAS instrument) for airborne nadir and limb measurements of atmospheric trace gases, liquid and solid water, and spectral radiances in the UV/vis and NIR spectral ranges. The spectrometer was developed for measurements from aboard the German High-Altitude and Long-Range (HALO) research aircraft during dedicated research missions. Here we report on the relevant instrumental details and the novel scaling method used to infer the mixing ratios of UV/vis absorbing trace gases from their absorption measured in limb geometry. The uncertainties of the scaling method are assessed in more detail than before for …

Atmospheric Science010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technology010502 geochemistry & geophysics01 natural sciencesUV/visible limb spectroscopylaw.inventionOpticslawErdsystem-Modellierungddc:550Nadirlcsh:TA170-171020701 environmental engineeringAbsorption (electromagnetic radiation)SpectroscopyScaling0105 earth and related environmental sciencesRemote sensingSpectrometerVerkehrsmeteorologielcsh:TA715-787business.industrylcsh:Earthwork. FoundationsAtmosphärische SpurenstoffeOptical spectrometerlcsh:Environmental engineeringTrace gasHALO mini-DOASEarth sciences13. Climate actionEnvironmental scienceHalobusinessAtmospheric Measurement Techniques
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Inter-comparison of stratospheric O<sub>3</sub> and NO<sub>2</sub> abundances retrieved from …

2006

Abstract. Stratospheric O3 and NO2 abundances measured by different remote sensing instruments are inter-compared: (1) Line-of-sight absorptions and vertical profiles inferred from solar spectra in the ultra-violet (UV), visible and infrared (IR) wavelength ranges measured by the LPMA/DOAS (Limb Profile Monitor of the Atmosphere/Differential Optical Absorption Spectroscopy) balloon payload during balloon ascent/descent and solar occultation are examined with respect to internal consistency. (2) The balloon borne stratospheric profiles of O3 and NO2 are compared to collocated space-borne skylight limb observations of the Envisat/SCIAMACHY satellite instrument. The trace gas profiles are retr…

Atmospheric Science010504 meteorology & atmospheric sciencesDifferential optical absorption spectroscopyBalloonAtmospheric sciences01 natural sciencesOccultationTrace gasSCIAMACHY010309 opticsAtmosphereAltitude13. Climate action0103 physical sciencesEnvironmental scienceSatellite0105 earth and related environmental sciencesRemote sensingAtmospheric Chemistry and Physics
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Evaluation of Disaggregation Methods for Downscaling MODIS Land Surface Temperature to Landsat Spatial Resolution in Barrax Test Site

2016

Thermal infrared (TIR) data are usually acquired at a coarser spatial resolution (CR) than visible and near infrared (VNIR). Several disaggregation methods have been recently developed to enhance the TIR spatial resolution using VNIR data. These approaches are based on the retrieval of a relation between TIR and VNIR data at CR, or training of a neural network, to be applied at the fine resolution afterward. In this work, different disaggregation methods are applied to the combination of two different sensors in the experimental test site of Barrax, Spain. The main objective is to test the feasibility of these techniques when applied to satellites provided with no TIR bands. Landsat and mod…

Atmospheric Science010504 meteorology & atmospheric sciencesMean squared errorNear-infrared spectroscopyTemperature0211 other engineering and technologies02 engineering and technology01 natural sciencesNormalized Difference Vegetation IndexVNIRRemote SensingSpectroradiometerImage resolutionImage enhancementLinear regressionEnvironmental scienceComputers in Earth SciencesImage resolution021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingDownscalingIEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
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The 2-μm spectroscopy of Huygens probe landing site on Titan with Very Large Telescope/Nasmyth Adaptive Optics System Near-Infrared Imager and Spectr…

2007

[1] Several ground-based telescopes followed the event of the Huygens probe descent through Titan's atmosphere (14 January 2005). We used the Nasmyth Adaptive Optics System Near-Infrared Imager and Spectrograph (NACO) adaptive optics system at the UT-4 of the Very Large Telescope in Chile to perform both spectroscopic and imaging measurements of Titan. We present here a selected sample of the spectra we acquired on 16 January 2005 in the K band between 2.03 and 2.40 μm. Our spectra include the Huygens landing site and surrounding dark and bright areas. We apply a radiative transfer code using new methane absorption coefficients calculated in the 2-μm region. The analysis of the data yields …

Atmospheric Science010504 meteorology & atmospheric sciencesSoil ScienceAquatic ScienceOceanography01 natural sciencesSpectral lineadaptive opticssymbols.namesakeOpticsGeochemistry and Petrology0103 physical sciencesEarth and Planetary Sciences (miscellaneous)Radiative transfersurfaceSpectroscopyAdaptive optics010303 astronomy & astrophysicsSpectrograph0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyPhysicsVery Large TelescopeEcology[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]business.industryNear-infrared spectroscopyPaleontologyForestryhaze[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Geophysics13. Climate actionSpace and Planetary Scienceradiative transferHuygenssymbolsbusinessTitan (rocket family)Titan
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2016

Abstract. Scanning spectrometer networks using scattered solar radiation in the ultraviolet spectral region have become an increasingly important tool for monitoring volcanic sulfur dioxide (SO2) emissions. Often measured spectra are evaluated using the differential optical absorption spectroscopy (DOAS) technique. In order to obtain absolute column densities (CDs), the DOAS evaluation requires a Fraunhofer reference spectrum (FRS) that is free of absorption structures of the trace gas of interest. For measurements at volcanoes such a FRS can be readily obtained if the scan (i.e. series of measurements at different elevation angles) includes viewing directions where the plume is not seen. I…

Atmospheric Science010504 meteorology & atmospheric sciencesSpectrometerbusiness.industryDifferential optical absorption spectroscopy010502 geochemistry & geophysicsResidual01 natural sciencesSpectral lineTrace gasPlumeOpticsPrincipal component analysisEnvironmental sciencebusinessZenith0105 earth and related environmental sciencesRemote sensingAtmospheric Measurement Techniques
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Adjusted Normalized Emissivity Method for surface temperature and emissivity retrieval from optical and thermal infrared remote sensing data

2003

[1] A methodology for the retrieval of surface temperatures and emissivities combining visible, near infrared and thermal infrared remote sensing data was applied to Digital Airborne Imaging Spectrometer (DAIS) data and validated with coincident ground measurements acquired in a multiyear experiment held in an agricultural site in Barrax, Spain. The Adjusted Normalized Emissivity Method (ANEM) is based on the use of visible and near infrared data to estimate the vegetation cover and model the maximum emissivity according to the Vegetation Cover Method. The pixel-dependent maximum emissivity is used as the initial guess of the Normalized Emissivity Method to obtain the surface temperature an…

Atmospheric ScienceAstrophysics::High Energy Astrophysical PhenomenaImaging spectrometerSoil ScienceDaisAstrophysics::Cosmology and Extragalactic AstrophysicsAquatic ScienceOceanographyStandard deviationGeochemistry and PetrologyCoincidentThermalEarth and Planetary Sciences (miscellaneous)EmissivityAstrophysics::Galaxy AstrophysicsEarth-Surface ProcessesWater Science and TechnologyRemote sensingEcologyCalor Radiació i absorcióNear-infrared spectroscopyPaleontologyForestryVegetationGeophysicsSpace and Planetary ScienceEnvironmental science
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In situ detection of atomic and molecular iodine using resonance and off-resonance fluorescence by lamp excitation: ROFLEX

2018

17 pags, 11 figs, 4 tabs

Atmospheric ScienceAtmospheric pressureAbsorption spectroscopylcsh:TA715-787Chemistrylcsh:Earthwork. FoundationsPhotodissociationAstrophysics::Instrumentation and Methods for AstrophysicsAnalytical chemistryResonanceFluorescencePhoton countinglcsh:Environmental engineeringExcited statelcsh:TA170-171Atomic physicsExcitation
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