0000000001177641

AUTHOR

S. Galeotti

showing 9 related works from this author

The data acquisition system for the ANTARES neutrino telescope

2006

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described.

Nuclear and High Energy Physics[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsData managementAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Data filteringData acquisition0103 physical sciences14. Life underwaterElectronics010306 general physicsInstrumentationdata acquisition system; neutrino telescopeRemote sensingAstroparticle physicsPhysicsneutrino telescope data acquisition system[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrino telescopedata acquisition systemComputer data storageFísica nuclearbusiness
researchProduct

The ANTARES Optical Beacon System

2007

ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirabl…

Nuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesneutrino telescope; optical beacon; time calibrationAstrophysics01 natural scienceslaw.inventionTelescope[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Opticslaw0103 physical sciencesCalibrationtime calibrationAngular resolution14. Life underwateroptical beacon010306 general physicsInstrumentationCherenkov radiationPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]neutrino telescope time calibration optical beacon010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeSITEAstronomyBeaconLIGHTFísica nuclearNeutrinobusiness
researchProduct

First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope

2006

In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The various data acquired during the continuous operation from April to December 2005 of the MILOM confirm the satisfactory performance of the Optical Modules, their front-end electronics and readout system, as well as the calibration devices of the detector. The in-situ measurement of the Optical Module time response yields a resolution better than 0.5 ns. The performance of the acoustic positioning system, which enables the spatial reconstruction of the ANTARES detector with a precision of about 10 cm, is verified. T…

Photomultiplierneutrino astronomy; photon detection; underwater detectorPositioning systemInstrumentationAstrophysics::High Energy Astrophysical PhenomenaNeutrino astronomy Underwater detector Photon detectionFOS: Physical sciencesAstrophysics01 natural sciencesneutrino astronomy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesCalibrationAngular resolution010306 general physicsRemote sensingAstroparticle physicsPhysicsunderwater detector[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomySITEAstronomy and AstrophysicsLIGHTPHOTON DETECTIONNEUTRINO ASTRONOMYFísica nuclearUNDERWATER DETECTORNeutrino astronomy
researchProduct

Management and Control of the Read Out Processors (tpps) of the Aleph Time Projection Chamber

1989

The readout of the Aleph time projection chamber (TPC) relies on a set of 72 time projection processors (TPPs), which are based on a Motorola 68020 microprocessor running a real-time operating system. The advanced processing capabilities of the TPPs allow them to perform in parallel a number of tasks, both during and outside of data acquisition, which are outlined. The management and control of such a large number of intelligent devices is presented. The discussion covers the hardware configuration of the TPPs; the software running the TPPs; their management, status, and control; exception handling and message logging; and the TPP monitoring tasks. >

Nuclear and High Energy PhysicsAlephTime projection chamberComputer sciencebusiness.industryException handlingElectrical engineeringlaw.inventionSet (abstract data type)MicroprocessorData acquisitionSoftwareNuclear Energy and EngineeringlawElectrical and Electronic EngineeringProjection (set theory)businessComputer hardware
researchProduct

The read-out processors of the Aleph time projection chamber and their performance

1990

The Aleph detector is installed on the LEP electron-positron storage ring. Its central tracking detector, a time projection chamber (TPC), has about 50000 channels of sampling electronics. The digitized signals are processed by 72 double-width Fastbus modules built around an MC 68020 processor. The time projection processor is described, and the solutions, both hardware and software, adopted to run and manage such a complex system in a Fastbus-VAX environment are discussed. Practical experience with the system is reported. >

PhysicsNuclear and High Energy PhysicsAlephTime projection chamberbusiness.industryDetectorElectrical engineeringTracking (particle physics)Particle detectorSoftwareNuclear Energy and EngineeringNuclear electronicsElectrical and Electronic EngineeringProjection (set theory)businessComputer hardwareIEEE Transactions on Nuclear Science
researchProduct

ALEPH: a Detector for Electron-Positron Annihilations at LEP

1990

Process-centred Software Engineering Environments (PSEE) are the most recent generation of environments supporting software development activities. Most of PSEE are based on mechanisms promoting enforcement and automation of process activities. In this kind of mechanisms the process models are prescribed in a detailed and complete way. But the experience shows that supporting processes is more concerned with the flexibility of guidance offered during the process performance than with enforcement of a collection of predefined process models. In this paper, we present a solution to support strategic processes in a PSEE by providing a flexible guidance during process enactment.

PhysicsFlexibility (engineering)Nuclear and High Energy PhysicsAlephhigh-energy physicsProcess modelingProcess (engineering)business.industrySoftware developmentLEPAutomationparticle detectorsData acquisitionDetectors and Experimental TechniquesLEP; particle detectors; high-energy physicsSoftware engineeringbusinessEnforcementInstrumentationparticle detector
researchProduct

The Monte San Nicola section (Sicily) revisited: A potential unit-stratotype of the Gelasian Stage

2022

The Monte San Nicola area (Southern Sicily) offers a spectacular exposure of open-marine sediments that were employed in 1998 for defining the Global Stratotype Section and Point (GSSP) of the Gelasian Stage (Upper Pliocene). After the lowering of the Pliocene/Pleistocene boundary to ca. 2.6 Ma in 2010, the Gelasian GSSP has been redefined as the base of both the Pleistocene Series and the Quaternary Period, which increased its importance and visibility within the scientific community. However, documentation on the Monte San Nicola reference section is still sparse. In the light of its renewed status, we decided to undertake a complete revision of the Gelasian Stage in its type area, in ord…

GSSPArcheologyGlobal and Planetary ChangeSettore GEO/02 - Geologia Stratigrafica E SedimentologicaStratigraphyPliocene-Pleistocene boundarymarine sedimentGeologySettore GEO/01 - Paleontologia E PaleoecologiaGelasianQuaternaryCalabrianmagnetostratigraphyEcology Evolution Behavior and Systematics
researchProduct

ANTARES: The first undersea neutrino telescope

2011

The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform neutrino astronomy and the apparatus also offers facilities for marine and Earth sciences. This paper describes the design, the construction and the installation of the telescope in the deep sea, offshore from Toulon in France. An illustration of the detector performance is given. © 2011 Elsevier B.V. All rights reserved.

Optical telescopesPhysics::Instrumentation and DetectorsAstronomyMarine engineeringSubmarine cablesAstrophysics01 natural scienceslaw.inventionAstroparticlelaw010303 astronomy & astrophysicsInstrumentationPhysicsDense wavelength division multiplexingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsSubmarine cableDeep seaNeutrino astronomyFísica nuclearNeutrinoMarine technologyAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Wet mateable connectorAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLINEOptical telescopePhysics::GeophysicsTelescopePhotomultiplier tube0103 physical sciencesNeutrinoDWDM14. Life underwaterDeep sea detectorInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORAstroparticle physics010308 nuclear & particles physicswet mateable connector.Marine technologyAstronomyElementary particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]PhotomultipliersKM3NeTFISICA APLICADAEarth (planet)High Energy Physics::ExperimentNeutrino astronomyastroparticle; neutrino astronomy; marine technology; dwdm; photomultiplier tube; deep sea detector; submarine cable; wet mateable connector; neutrinoSYSTEMTelescopes
researchProduct

Direct measurement of the W boson width

2009

We present a direct measurement of the width of the W boson using the shape of the transverse mass distribution of W->enu candidates selected in 1 fb-1 of data collected with the D0 detector at the Fermilab Tevatron collider in ppbar collisions at sqrt{s}=1.96 TeV. We use the same methods and data sample that were used for our recently published W boson mass measurement, except for the modeling of the recoil, which is done with a new method based on a recoil library. Our result, 2.028 +- 0.072 GeV, is in agreement with the predictions of the standard model.

Particle physicsTevatronGeneral Physics and AstronomyFOS: Physical sciences= 1.8 TEVElementary particle01 natural sciencesHigh Energy Physics - ExperimentStandard Modellaw.inventionNuclear physicsCOLLIDERParticle decayHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)RecoilRATIOPBARP COLLISIONSlaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSFermilabCollider010306 general physicsNuclear ExperimentBosonPhysics010308 nuclear & particles physicsComputer Science::Information Retrieval14.70.Fm 13.38.Be 13.85.QkTransverse mass= 1.8 TEV; PBARP COLLISIONS; RADIATIVE-CORRECTIONS; RATIO; COLLIDER; DECAYHigh Energy Physics::ExperimentCollider Detector at FermilabDECAY
researchProduct