Search results for "PHOTOMULTIPLIER"

showing 10 items of 194 documents

FPGA based digital lock-in amplifier for fNIRS systems

2018

Lock-In Amplifiers (LIA) represent a powerful technique helping to improve signals detectability when low signal to noise ratios are experienced. Continuous Wave functional Near Infrared Spectroscopy (CW-fNIRS) systems for e-health applications usually suffer of poor detection due to the presence of strong attenuations of the optical recovering path and therefore small signals are severely dipped in a high noise floor. In this work a digital LIA system, implemented on a Zynq® Field Programmable Gate Array (FPGA), has been designed and tested to verify the quality of the developed solution, when applied in fNIRS systems. Experimental results have shown the goodness of the proposed solutions.

010302 applied physicsComputer scienceAmplifier0206 medical engineeringLock-in amplifierDigital lock-in amplifier02 engineering and technology020601 biomedical engineering01 natural sciencesNoise floorSettore ING-INF/01 - ElettronicaSilicon photomultiplier (SiPM)Quality (physics)0103 physical sciencesElectronic engineeringContinuous waveFunctional near-infrared spectroscopyField-programmable gate arrayFpgaFunctional near-infrared spectroscopy
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Design and implementation of PET detectors based on monolithic crystals and SiPMs

2018

Esta tesis doctoral se centra tanto en el diseño como en la validación experimental de detectores de rayos gamma para escáneres de tomografía por emisión de positrones (PET, del inglés Positron Emission Tomography). El objetivo principal de esta tesis es el diseño de innovadores bloques detectores PET de alto rendimiento. La técnica PET constituye una de las principales herramientas diagnósticas en medicina nuclear, que es una especialidad médica que utiliza sustancias radiactivas con fines diagnósticos y terapéuticos. Esta técnica de imagen médica permite visualizar procesos fisiológicos y bioquímicos del cuerpo humano in vivo, mediante la administración del elemento radiotrazador. Los rad…

240606 Física MédicaMonolithic blockPositron emission tomography (PET)Depth of interaction (DOI)Medical imagingSilicon photomultiplierMagnetic resonance (MRI)
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SiPM based tracking for detector calibration in NEXT

2015

197 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear de la Universidad de Valencia y del Instituto de Física Corpuscular (IFIC).

:FÍSICA::Otras especialidades físicas [UNESCO]Xenon Gas DetectorsExperimento NEXTModelo StandardSilicon PhotoMultipliersFísica de PartículasUNESCO::FÍSICA::Otras especialidades físicasNeutrinoless Double Beta Decay
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Fast photon detection for particle identification with COMPASS RICH-1

2006

Particle identification at high rates is an important challenge for many current and future high-energy physics experiments. The upgrade of the COMPASS RICH-1 detector requires a new technique for Cherenkov photon detection at count rates of several $10^6$ per channel in the central detector region, and a read-out system allowing for trigger rates of up to 100 kHz. To cope with these requirements, the photon detectors in the central region have been replaced with the detection system described in this paper. In the peripheral regions, the existing multi-wire proportional chambers with CsI photocathode are now read out via a new system employing APV pre-amplifiers and flash ADC chips. The ne…

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsCherenkov detectorOther Fields of PhysicsFOS: Physical sciencesCOMPASS; RICH; Multi-anode PMT; Particle identificationCOMPASSParticle identificationPhotocathodelaw.inventionParticle identificationNuclear physicsOpticsMulti-anode PMTlawCompassCOMPASS; RICHInstrumentationRICHCherenkov radiationPhysicsbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)UpgradePhysics - Accelerator PhysicsHigh Energy Physics::Experimentbusiness
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The IceCube prototype string in Amanda

2006

The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole Station. Each OM contains a photomultiplier tube (PMT) that detects photons of Cherenkov light generated in the ice by muons and electrons. IceCube is a cubic-kilometer-sized expansion of Amanda currently being built at the South Pole. In IceCube the PMT signals are digitized already in the optical modules and transmitted to the surface. A prototype string of 41 OMs equipped with this new all-digital technology was deployed in the Amanda array in the year 2000. In this paper we describe the technology and demonst…

Antarctic Muon And Neutrino Detector ArrayAstroparticle physicsPhysicsNuclear and High Energy PhysicsPhotomultiplierPhotonMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Neutrino telescopeAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysicsNeutrino telescopeAmandaIceCubeData acquisitionSignal digitizationAmanda; IceCube; Neutrino telescope; Signal digitizationInstrumentationCherenkov radiation
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First year performance of the IceCube neutrino telescope

2006

The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence…

Astroparticle physicsPhysicsPhotomultiplierMuonPerformanceDetectorAstrophysics (astro-ph)AstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsIceCube Neutrino ObservatoryAmandaIceCubeDetectionData acquisitionFirst yearAmanda; Detection; First year; IceCube; IceTop; Neutrino; Performance; South poleNeutrinoSouth poleAstronomiaIceTopNeutrinoCherenkov radiation
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Position-sensitive neutron detector

2002

Abstract A position-sensitive neutron detector has been developed for use in nuclear physics research. The detector consists of a ∅5.5 cm×100 cm long quartz tube filled with liquid scintillator viewed from both ends by photomultipliers and enclosed in a light-tight titanium container. The properties of the detector were determined both experimentally and by Monte Carlo simulations (EFEN code). A time resolution of 0.4 ns was reached resulting in the position resolution of less than 4 cm. The neutron registration efficiency varies from 36% to 20% within neutron energy range 1–10 MeV and is practically independent of the position along the detector length. Good n–γ separation is achieved for …

Bonner spherePhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectorsbusiness.industryNuclear TheoryMonte Carlo methodDetectorScintillatorNeutron temperatureNuclear physicsOpticsNeutron detectionNeutronNuclear ExperimentbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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CY5 fluorescence measured with silicon photomultipliers

2014

This paper presents an efficient optical biosensor set up for a low-level light detection, using fluorescent dyes and a novel Si-based detector. Fluorescence emitted by a traditional fluorophore, CY5, widely used as optical label in DNA microarrays, was detected using a 25 pixels Silicon photomultiplier (SiPM), a device formed by avalanche diodes operating in Geiger mode, in parallel connections. We measured the fluorescence current in different deposition (fluorophore concentration; solvent; salt concentration) and operation (angle of analysis, optical laser power, device gain) conditions. The characterization of DNA samples labeled with CY5 is also reported to demonstrate the detector pot…

DNA recognitionMaterials sciencebusiness.industrySiPMtechnology industry and agricultureFluorescenceeye diseasesfluorescence detectorCY5OpticsSilicon photomultiplierOptoelectronicsbusinessCY5; DNA recognition; fluorescence detector; optical transduction; SiPMoptical transduction
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SiPM as miniaturised optical biosensor for DNA-microarray applications

2015

A miniaturized optical biosensor for low-level fluorescence emitted by DNA strands labelled with CY5 is showed. Aim of this work is to demonstrate that a Si-based photodetector, having a low noise and a high sensitivity, can replace traditional detection systems in DNA-microarray applications. The photodetector used is a photomultiplier (SiPM), with 25 pixels. It exhibits a higher sensitivity than commercial optical readers and we experimentally found a detection limit for spotted dried samples of ∼1 nM. We measured the fluorescence signal in different operating conditions (angle of analysis, fluorophores concentrations, solution volumes and support). Once fixed the angle of analysis, for s…

Detection limitAnalytePhotomultiplierMaterials scienceoptical biosensorbusiness.industrySiPMDNA microarrayPhotodetectorLinearityDNA-microarraySignalSettore ING-INF/01 - ElettronicaElectronic Optical and Magnetic MaterialsSilicon photomultiplierOpticslcsh:TA1-2040DNA microarray; Fluorophore detection; Optical Biosensor; SiPMSignal ProcessingElectrical and Electronic Engineeringbusinesslcsh:Engineering (General). Civil engineering (General)Sensitivity (electronics)Fluorophore detectionBiotechnologySensing and Bio-Sensing Research
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