0000000000660427

AUTHOR

Stefano Cecchini

showing 2 related works from this author

Time calibration of the ANTARES neutrino telescope

2011

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described.

Optical telescopesPhysics - Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectors01 natural sciencesOptimal performanceHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Calibration procedureDimensional arraysAngular resolution[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino energyNEUTRINO TELESCOPE010303 astronomy & astrophysicsPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)Deep seaNeutrino detectorRelative timeCalibrationFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsTime calibrationPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov lightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesScattering lengthNeutrino TelescopesOptical telescopeNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Tellurium compounds0103 physical sciencesOptical systemsCalibrationAngular resolution14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORCherenkov radiationtime calibration; neutrino telescopes; antaresANTARES010308 nuclear & particles physicsNeutrino interactionsAstronomyElementary particlesAstronomy and AstrophysicsPhotomultipliersFISICA APLICADAHigh Energy Physics::ExperimentUNDERWATER DETECTORNeutrino telescopesSYSTEM
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Effects of Sulla forage (Sulla coronarium L.) on the oxidative status and milk polyphenol content in goats

2015

Abstract Twelve milking Girgentana goats were allocated into 3 groups and fed 3 diets ad libitum in a 3 × 3 Latin square design with 3 periods. The diets were Sulla fresh forage ad libitum (SUL), Sulla fresh forage ad libitum and 800 g/d of barley meal (SULB), and mixed hay ad libitum and 800 g/d of barley meal (HB). Changes were observed in total polyphenol intake, plasma oxidative status, plasma polyphenol content, metabolic status, milk polyphenol content, and total antioxidant capacity. The fresh forage diets (SUL and SULB) increased dry matter, total polyphenol, nontannic polyphenol and tannin intakes, and the milk total protein, casein, milk total polyphenols, and milk free polyphenol…

Settore AGR/19 - Zootecnica SpecialeAntioxidantSulla foragemedicine.medical_treatmentoxidative status; milk; Sulla forage; polyphenolAntioxidantsCaseinGeneticsmedicineTanninAnimalsLactationDry matterFood sciencechemistry.chemical_classificationMealmilkChemistryGoatsfood and beveragesPolyphenolsFabaceaeHordeumoxidative statuMilk ProteinsAnimal FeedDietpolyphenolProanthocyanidinPolyphenolHayAnimal Science and ZoologyFemaleEnergy MetabolismTanninsFood Science
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