Search results for "Instrumentation"

showing 10 items of 4914 documents

Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)

2022

International audience; A new generation magnetic spectrometer in space will open the opportunity to investigate the frontiers in direct high-energy cosmic ray measurements and to precisely measure the amount of the rare antimatter component in cosmic rays beyond the reach of current missions. We propose the concept for an Antimatter Large Acceptance Detector In Orbit (ALADInO), designed to take over the legacy of direct measurements of cosmic rays in space performed by PAMELA and AMS-02. ALADInO features technological solutions conceived to overcome the current limitations of magnetic spectrometers in space with a layout that provides an acceptance larger than 10 m sr. A superconducting ma…

antimatter; cosmic rays; dark matter; particle detectors; space instrumentation;space instrumentationcosmic raysantimatter; cosmic rays; dark matter; particle detectors; space instrumentationAstrophysics::High Energy Astrophysical PhenomenaSettore FIS/01 - Fisica Sperimentaleantimatter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]particle detectorsInstrumentationdark mattercosmic rays; antimatter; dark matter; particle detectors; space instrumentation
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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In Vitro Antioxidant Activity and In Vivo Topical Efficacy of Lipid Nanoparticles Co-Loading Idebenone and Tocopheryl Acetate

2019

Idebenone (IDE) is a strong antioxidant that has been proposed for the treatment of skin disorders, including skin ageing. Unfavorable physico-chemical properties make IDE a poor skin permeant where effectiveness could be improved by its loading into suitable delivery systems such as solid lipid nanoparticles (SLN) and nanostructured lipid carriers (NLC). In this work, we designed novel IDE-loaded NLC containing tocopheryl acetate (VitE) as a liquid component to obtain a synergic effect between IDE and VitE. The resulting NLC showed small particle sizes (24&ndash

antioxidantAntioxidantDPPHmedicine.medical_treatment02 engineering and technologylipid nanoparticlesPharmacologytocopheryl acetatemedicine.disease_causelcsh:Technology030226 pharmacology & pharmacylcsh:Chemistry03 medical and health scienceschemistry.chemical_compoundphoto-protective effect0302 clinical medicineIn vivoSolid lipid nanoparticlemedicineIdebenoneGeneral Materials Scienceskin hydrationlcsh:QH301-705.5InstrumentationFluid Flow and Transfer ProcessesIdebenonelcsh:TChemistryProcess Chemistry and TechnologyGeneral EngineeringIn vitro toxicologytopical administrationlipid nanoparticle021001 nanoscience & nanotechnologylcsh:QC1-999kin hydrationComputer Science Applicationsantioxidantslcsh:Biology (General)lcsh:QD1-999Idebenone; tocopheryl acetate; lipid nanoparticles; antioxidants; topical administration; skin hydration; photo-protective effectlcsh:TA1-2040Tocopheryl acetatelcsh:Engineering (General). Civil engineering (General)0210 nano-technologylcsh:PhysicsOxidative stressmedicine.drugApplied Sciences
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Species-Specific Antioxidant Power and Bioactive Properties of the Extracts Obtained from Wild Mediterranean Calendula Spp. (Asteraceae)

2019

In this study we focused on four taxa of the genus Calendula (C. maritima, C. suffruticosa subsp. fulgida, C. arvensis, and the hybrid between the first two ones), collected in Mediterranean area (Sicily). Six extracts for each species were obtained using solvents with increasing polarity (hexane, ethanol 80%, acetone 70%, and water) and through extraction by supercritical fluids (SFE). It has been observed that the solvent with the highest extraction efficiency was ethanol 80% for all species. However, SFE extracts showed high antioxidant activity comparable to the ethanol 80% extract (polyphenol, DPPH, and reducing power method). These findings were confirmed by in vitro analysis (MTT ass…

antioxidantAntioxidantDPPHmedicine.medical_treatmentcalendula specielcsh:Technology01 natural scienceslcsh:Chemistrystresschemistry.chemical_compoundSettore BIO/10 - BiochimicaGeneral Materials ScienceFood scienceSettore BIO/06 - Anatomia Comparata E CitologiaCalendulalcsh:QH301-705.5InstrumentationFluid Flow and Transfer Processes0303 health sciencesbiologyplantsGeneral EngineeringSupercritical fluid extractionlcsh:QC1-999Computer Science ApplicationsSolventantioxidantscalendula speciesopuntia-ficus-indica03 medical and health sciencesmedicineAcetoneby-productspolyphenols030304 developmental biologylcsh:TACLProcess Chemistry and TechnologyExtraction (chemistry)assaybiology.organism_classification0104 chemical sciences010404 medicinal & biomolecular chemistrylcsh:Biology (General)lcsh:QD1-999chemistrylcsh:TA1-2040PolyphenolbioactivitySettore BIO/03 - Botanica Ambientale E Applicataflavonoidsmarigoldsupercritical fluid extraction[SDE.BE]Environmental Sciences/Biodiversity and Ecologylcsh:Engineering (General). Civil engineering (General)lcsh:Physicsphenolic compositionApplied Sciences
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Synergistic enhancement via plasmonic nanoplate-bacteria-nanorod supercrystals for highly efficient SERS sensing of food-borne bacteria

2017

Bio-sensing techniques utilizing metallic nanoparticles as a probe have gained more and more attention and play today an important role in the detection of bacteria. To date, although several sensing materials have been tested, there is still a long way to go to achieve a fast, low-cost, ultrasensitive and multifunctional substrate suitable for a universal biosensor for detection of bacterial cells. Here, we report a novel probe design based on anisotropic plasmonic nanoparticles organized to a biocompatible 3D bio-inorganic scaffold, i.e., nanoplate-bacteria-nanorod supercrystals (NBNS) with extremely high surface-enhanced Raman spectroscopic (SERS) activity as a model of synergistic plasm…

assemblyMaterials scienceta221NanoparticleNanotechnology02 engineering and technologyrecognition of microbes010402 general chemistry01 natural sciencesBiokemia solu- ja molekyylibiologia - Biochemistry cell and molecular biologybakteeritsymbols.namesakeNanoteknologia - NanotechnologyMaterials ChemistryKemia - Chemical sciencesElectrical and Electronic EngineeringbacteriaInstrumentationPlasmonPlasmonic nanoparticlesmikrobien tunnistaminenta114SERSMetals and AlloysSubstrate (chemistry)021001 nanoscience & nanotechnologyCondensed Matter Physicschemometrics0104 chemical sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialsasymmetric nanoparticlessymbolsnanoparticlesNanorodnanopartikkelit0210 nano-technologyRaman spectroscopyBiosensorRaman scattering
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Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX

2020

We present the first detection of atomic emission lines from the atmosphere of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq $\sim$ 4, 000 K). We combined thousands of spectrally resolved lines observed during one night with the HARPS-N spectrograph (R $\sim$ 115, 000), mounted at the Telescopio Nazionale Galileo. We introduce a novel statistical approach to extract the planetary parameters from the binary mask cross-correlation analysis. We also adapt the concept of contribution function to the context of high spectral resolution observations, to identify the location in the planetary atmosphere where the detected emission originates. The average planetary li…

astro-ph.SR010504 meteorology & atmospheric sciencesContinuum (design consultancy)FOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesExoplanet atmospheres; Exoplanet atmospheric composition; High resolution spectroscopyAtmosphereHigh resolution spectroscopy0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumSpectral resolution010303 astronomy & astrophysicsSpectrographInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Settore FIS/05Astronomy and AstrophysicsExoplanetAstrophysics - Solar and Stellar AstrophysicsExoplanet atmospheric composition13. Climate actionSpace and Planetary Scienceastro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresastro-ph.IM
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The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
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Search for cosmic sources in neutrino telescopes and time calibration in the ANTARES neutrino telescope

2018

Aunque la astronomía de neutrinos es una disciplina muy reciente, está resultando ser muy en un estado estimulante. Los diversos resultados publicados por la colaboración IceCube han mostrado la existencia de un flujo de neutrinos cósmicos de altas energías, del cual se desconoce su origen, y del que no se ha observado una dirección privilegiada. El telescopio de neutrinos ANTARES ha sido capaz de excluir la posibilidad de que algunos de los eventos observados por IceCube se hayan producido por una fuente puntual en la región del centro galáctico. Además, el último análisis de flujos difusos de ANTARES muestra un resultado compatible con el flujo observado por IceCube. Actualmente, existen …

astronomyneutrinoANTARES:FÍSICA [UNESCO]Astrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopesUNESCO::FÍSICAUNESCO::ASTRONOMÍA Y ASTROFÍSICA:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]IceCube
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Towards high-accuracy mass spectrometry of highly charged short-lived ions at ISOLTRAP

2006

Dedicated to H.-J. Kluge on the occasion of his 65th birthday anniversary - Jürgen Kluge Special Issue; Multiply charged ions of stable xenon isotopes from a plasma ion source have been mass-selected by the on-line mass separator ISOLDE/CERN and delivered to the triple-trap mass spectrometer ISOLTRAP. The doubly charged ions that survived the charge-exchange processes during bunching and ion preparation were transferred to a precision Penning trap for mass determination. Mass values were obtained for the isotopes with mass numbers A=126,129,130,136. They are consistent with previous results except for the case of $^{126}Xe$ where a significant deviation from the literature value was found. …

atomic masses[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Thermal ionization mass spectrometryMass spectrometry01 natural sciencesISOLTRAPhistory of atomic massesNuclear physics0103 physical scienceshistory of mass spectrometryPhysical and Theoretical ChemistryNuclear Experiment010306 general physicsInstrumentationQuadrupole mass analyzerSpectroscopy010308 nuclear & particles physicsChemistryNuclear binding energiesHighly charged ionevaluation of atomic massesCondensed Matter PhysicsPenning trapIon sourceAtomic physicsHybrid mass spectrometerInternational Journal of Mass Spectrometry
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