Search results for " Detection"

showing 10 items of 1676 documents

Detecting gravitational waves from cosmological phase transitions with LISA: an update

2020

MC was funded by the Royal Society under the Newton International Fellowship program. GD would like to thank CNPq (Brazil) for financial support. MH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1), and the Academy of Finland (grant number 286769). SJH was supported by the Science and Technology Facilities Council (grant number ST/P000819/1). The work of JK was supported by Department of Energy (DOE) grant DE-SC0019195 and NSF grant PHY-1719642. TK and GS are funded by the Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy - EXC 2121 \Quantum Universe" - 390833306. JMN is supported by Ramon y Cajal Fellowship contract RYC-2017-22986…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterstandard modelFOS: Physical sciencesContext (language use)gravitational radiation: direct detection01 natural sciencesdark matterbubble: nucleationGravitational wavesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciencesEffective field theoryenergy: densitynumerical calculationsCosmological phase transitionsperturbation theoryPhysics:Matematikk og Naturvitenskap: 400::Fysikk: 430 [VDP]wave: acousticLISACOSMIC cancer database010308 nuclear & particles physicsGravitational wavenew physicsGravitational theorygravitational radiationAstronomy and Astrophysicscritical phenomenagravitational radiation detectorHigh Energy Physics - PhenomenologyGravitational sourcesgravitational radiation: emission[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs modelPerturbation theory (quantum mechanics)gravitational radiation: power spectrum[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]dilatonAstrophysics - Cosmology and Nongalactic Astrophysics
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Novel Immune TiO2 Photoluminescence Biosensors for Leucosis Detection

2012

Abstract Novel immune photoluminescent biosensor, based on TiO2 nanoparticles, for retroviral leucosis detection has been developed. The photoluminescence spectra were excited by solid state laser with wavelength 355 nm and measured in the range of 370-800 nm. Original photoluminescence spectrum of TiO2 nanoparticles showed wide maximum at 515 nm. The biosensitive layer was formed by immobilization of retroviral leucosis antigens on the surface of TiO2 nanoparticles. Immobilization of antigens on TiO2 surface led to UV-shift of photoluminescence spectrum and increase of PL intensity. The response to different concentrations of retroviral leucosis antibodies has been measured. The decrease o…

PhotoluminescenceMaterials scienceTio2 nanoparticlesAnalytical chemistryleucosis detectionGeneral MedicinePhotochemistryLeucosisimmune biosensorsAdsorptionImmune systemExcited statephotoluminescenceBiosensorEngineering(all)TiO2 nanostructuresProcedia Engineering
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The fast photon detection system of COMPASS RICH-1

2007

Abstract A fast photon detection system has been built for the upgrade of COMPASS RICH-1, the large size gaseous RICH detector in use at the COMPASS Experiment at the CERN SPS since 2001. The photon detectors of the central region have been replaced by a new system based on multi-anode photomultipliers coupled to individual fused silica lens telescopes and a fast readout electronics system, while in the outer region the existing MWPCs with CsI photocathodes have been equipped with a new readout system, based on the APV chip. RICH-1 has been successfully operated in its upgraded version during the 2006 run. We report on the upgrade design and construction, and on the preliminary characteriza…

PhotomultiplierNuclear and High Energy PhysicsPhotonMulti-anode photomultiplier tubesPhysics::Instrumentation and DetectorsUV lensesCOMPASS; Multi-anode photomultiplier tubes; Photon detection; RICH; UV lenses; Nuclear and High Energy Physics; InstrumentationCOMPASSlaw.inventionFAST-RICH; DEUTERON; READOUT; DESIGNOpticsDESIGNlawMulti-anode photomultiplier tubeCompassCOMPASS experimentRICHInstrumentationNuclear and High Energy PhysicPhysicsLarge Hadron Colliderbusiness.industryDetectorREADOUTDEUTERONLens (optics)UpgradePhoton detectionFAST-RICHUV lenseHigh Energy Physics::Experimentbusiness
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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
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Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22

2019

We present a multi-band search for X-ray, optical and $\gamma$-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations, performed in 2005 and 2014, at a luminosity of $\sim$2-3$\times$10$^{30}$ erg s$^{-1}$, in the 0.5-8 keV energy range. The radio and the X-ray source positions are found consistent within 1$\sigma$ error box. No detection is found in archival XMM-Newton and Swift/XRT observations, compatible with the Chandra flux level. The low statistics prevents us to assess if the X-ray source varied between the two observations. The X-ray spectrum is consistent with a power…

PhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminosityX-rays: binariesMillisecond pulsarpulsars: general0103 physical sciences010303 astronomy & astrophysicsX-rays: individual: PSR J1836-2354AAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsglobular clusters: individual: M22 (NGC 6656)Astronomy and AstrophysicsX-rays: binarie13. Climate actionSpace and Planetary ScienceGlobular clusterNo detectionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Real-time and low-cost sensing technique based on photonic bandgap structures

2011

[EN] A technique for the development of low-cost and high-sensitivity photonic biosensing devices is proposed and experimentally demonstrated. In this technique, a photonic bandgap structure is used as transducer, but its readout is performed by simply using a broadband source, an optical filter, and a power meter, without the need of obtaining the transmission spectrum of the structure; thus, a really low-cost system and real-time results are achieved. Experimental results show that it is possible to detect very low refractive index variations, achieving a detection limit below 2 x 10(-6) refractive index units using this low-cost measuring technique. (C) 2011 Optical Society of America[

PhotonsTime FactorsMaterials sciencebusiness.industrySensorsWave-GuidesOptical DevicesPhysics::OpticsSodium ChlorideSlow lightAtomic and Molecular Physics and OpticsSlow-LightOpticsTransducerTransmission (telecommunications)Fiber Bragg gratingLimit of DetectionBroadbandTEORIA DE LA SEÑAL Y COMUNICACIONESOptoelectronicsBiosensor ArrayPhotonicsOptical filterbusinessRefractive index
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Quantum dots functionalised artificial peptides bioinspired to the D1 protein from the Photosystem II of Chlamydomonas reinhardtii for endocrine disr…

2021

Herein we describe the design and synthesis of novel artificial peptides mimicking the plastoquinone binding niche of the D1 protein from the green photosynthetic alga Chlamydomonas reinhardtii, also able to bind herbicides. In particular, molecular dynamics (MD) simulations were performed to model in silico the behaviour of three peptides, D1Pep70-H, D1Pep70-S264K and D1Pep70-S268C, as genetic variants with different affinity towards the photosynthetic herbicide atrazine. Then the photosynthetic peptides were functionalised with quantum dots for the development of a hybrid optosensor for the detection of atrazine, one of the most employed herbicides for weed control in agriculture as well …

Photosystem IIIn silicoChlamydomonas reinhardtiiPlastoquinone02 engineering and technologyEndocrine DisruptorsPhotosynthesis01 natural sciencesOptosensorAnalytical Chemistrychemistry.chemical_compoundBiomimetic peptidesbiomimeticsAtrazineSettore CHIM/02 - Chimica FisicabiologyHerbicidesQuantum dots010401 analytical chemistryherbicide detectionPhotosystem II Protein Complexbiosensors021001 nanoscience & nanotechnologybiology.organism_classification0104 chemical sciencesEndocrine disruptorchemistryQuantum dotSettore CHIM/03 - Chimica Generale E InorganicaBiophysicsAtrazinePeptides0210 nano-technologyChlamydomonas reinhardtii
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Syntax Error Handling

1990

In the previous chapters we have seen that the various parsers discussed, at least whenever they are deterministic, detect an error in any nonsentence. This means, that on any nonsentence there is a computation ending with an error configuration. For practical parsers, mere error detection is not enough; the parser should also emit a meaningful error message and recover from the error. A recovery means that the error configuration is transformed into a non-error configuration at which normal parsing can be resumed. Moreover, the transformation should be done so that as few input symbols as possible will be discarded. The goal of the error recovery is to maximize the amount of input text tha…

PhraseParsingComputer sciencemedia_common.quotation_subjectComputationAmbiguitycomputer.software_genreTransformation (function)Quality (business)Syntax errorError detection and correctionAlgorithmcomputermedia_common
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The analog Resistive Plate Chamber detector of the ARGO-YBJ experiment

2015

The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the YangBaJing Cosmic Ray Observatory (4300 m a.s.l.). The detector consists of a single layer of Resistive Plate Chambers (RPCs) (6700 m2) operated in streamer mode. The signal pick-up is obtained by means of strips facing one side of the gas volume. The digital readout of the signals, while allows a high space–time resolution in the shower front reconstruction, limits the measurable energy to a few hundred TeV. In order to fully investigate the 1–10 PeV region, an analog readout has been implemented by instrumenting each RPC with two large size electrodes facing the other side of the gas volume…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAir shower detectionFOS: Physical sciencesCosmic raySTRIPSCalorimetrySignallaw.inventionOpticsObservatorylawAir shower detection RPC detector CalorimetryCosmic-ray observatoryphysics.ins-detInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsResistive touchscreenbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Core (optical fiber)RPC detectorbusinessAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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PINGU: a vision for neutrino and particle physics at the South Pole

2017

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60,000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters $\theta_{\rm 23}$ and $\Delta m^2_{\rm 32}$, including the octan…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmixing [neutrino]atmospheric neutrinos; IceCube Neutrino Observatory; neutrino oscillations; PINGU; Nuclear and High Energy Physicspole7. Clean energy01 natural sciencesPINGUIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - ExperimentObservatoryPhysicssolar [WIMP]precision measurementAstrophysics::Instrumentation and Methods for Astrophysicsoscillation [neutrino]solar [dark matter]atmosphere [neutrino]threshold [energy]mass difference [neutrino]atmospheric neutrinosobservatoryHigh Energy Physics - PhenomenologyUpgradeNeutrino detectorupgradeNeutrinoKM3NETperformanceParticle physicsNuclear and High Energy Physicssupernova [neutrino]particle identification [neutrino/tau]Astrophysics::High Energy Astrophysical PhenomenaSUPERNOVA DETECTIONIceCube Neutrino Observatory0103 physical sciencesOSCILLATIONSmass: low [dark matter]unitarityddc:530010306 general physicsNeutrino oscillationneutrino oscillations010308 nuclear & particles physicsAstronomysensitivityKM3NeTPhysics and Astronomymass [neutrino]beam [neutrino]High Energy Physics::ExperimentgalaxyATMOSPHERIC NEUTRINOSMATTERSYSTEMLeptonmixing angle [neutrino]experimental results
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