Search results for "ANTARES NEUTRINO TELESCOPE"

showing 5 items of 5 documents

Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

2013

The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in th…

:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]0106 biological sciencesDYNAMICSSalinityANTARES NEUTRINO TELESCOPE010504 meteorology & atmospheric sciencesNaturwissenschaftliche Fakultät -ohne weitere Spezifikation-IMPACTOcean CirculationPsychologie appliquéelcsh:MedicineCell CountAstronomical SciencesOceanografiaAstrophysicsOceanographyEcologia marina01 natural sciencesBathyal zoneNEUTRINO TELESCOPESMediterranean seaOceanslcsh:Sciencedeep-sea bioluminescenceantaresEcosistemes marinsMultidisciplinaryCLIMATE-CHANGEEcologyMediterrània (Mar)Mediterranean RegionEcologyMarine EcologyMEDITERRANEAN SEAEutrophicationBiogeochemistrySciences bio-médicales et agricolesDeep seaANTARES NEUTRINO TELESCOPE; MEDITERRANEAN SEA; INTERANNUAL VARIABILITYOceanographyLight emissionSeasonsddc:500BioluminescenceINTERANNUAL VARIABILITYBiologieResearch ArticleATLANTICGULFOceans and Seas[PHYS.PHYS.PHYS-BIO-PH]Physics [physics]/Physics [physics]/Biological Physics [physics.bio-ph]Marine Biology-ConvectionDeep seaFluorescenceMicrobial EcologyCarbon CycleMarine ecologyAstroparticle PhysicsMediterranean SeaAnimalsWater ColumnEcosystemSeawater14. Life underwaterSalinitatNeutrinosBiology[SDU.STU.OC]Sciences of the Universe [physics]/Earth Sciences/Oceanography0105 earth and related environmental sciencesMarine planktonBACKGROUND LIGHT010604 marine biology & hydrobiologyBiological Oceanographylcsh:RPlànctonPelagic zoneMarine and aquatic sciencesEarth sciencesLight intensitySea waterGeochemistry13. Climate actionCONVECTIONFISICA APLICADALuminescent MeasurementsAigua de marEnvironmental sciencelcsh:QEutrophicationPhysical Oceanography
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A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsRayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesantaresAstrophysicsddc:500.2Neutrino fluxesGamma ray burstsPartícules (Física nuclear)law.inventionTelescopeneutrinoRaigs gammalaw14. Life underwaterNeutrinsNeutrinosEngineering (miscellaneous)Cherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayfermi bubbles; antares; neutrinoDetectorCharged particleNeutrino astrophysicsFermi bubbleneutrino telecope13. Climate actionFermi bubblesCol·lisions (Física nuclear):Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAntares neutrino telescopeFermi Gamma-ray Space Telescope
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A search for time dependent neutrino emission from microquasars with the ANTARES telescope

2014

[EN] Results are presented on a search for neutrino emission from a sample of six microquasars, based on the data collected by the ANTARES neutrino telescope between 2007 and 2010. By means of appropriate time cuts, the neutrino search has been restricted to the periods when the acceleration of relativistic jets was taking place at the microquasars under study. The time cuts have been chosen using the information from the X-ray telescopes RXTE/ASM and Swift/BAT, and, in one case, the gamma-ray telescope Fermi/LAT. No statistically significant excess has been observed, thus upper limits on the neutrino fluences have been derived and compared to the predictions by models. Constraints have bee…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminositylaw.inventionTelescopeneutrinoAstrophysical jetlawMicroquasars0103 physical sciencesmicroquasarNeutrinos010303 astronomy & astrophysicsAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyFísicaAstronomy and AstrophysicsSolar neutrino problemNeutrino detectorSpace and Planetary ScienceFISICA APLICADANuclear and High Energy Physics; Astronomy and Astrophysics; Space and Planetary ScienceHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaANTARES neutrino telescopeFermi Gamma-ray Space Telescope
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Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

2011

An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170 m above the sea bed at 2475 m. The ADCP measured downward vertical currents of magnitudes up to 0.03 m s-1 in late winter and early spring 2006. In the same period, observations were made of enhanced levels of acoustic reflection, interpreted as suspended particles including zooplankton, by a factor of about 10 and of horizontal currents reaching 0.35 m s-1. These observations coincided with high light levels detected by the telescope, interpreted …

Optical telescopesDense water formation010504 meteorology & atmospheric sciencesDense watersBoundary currentWave reflectionOptical photo-multiplier observationsSuspended loadWATER FORMATIONOceanography01 natural scienceslaw.inventionPhysics - GeophysicsObservational methodMediterranean sea86-02lawDeep MediteraneanSeabedPhosphorescenceDeep seaCurrent (stream)VARIABILITYOptical methodOceanographyAcoustic variables measurementNorthern boundary currentantares neutrino telescope; deep mediteranean; northern boundary current; acoustic adcp observations; episodic downward current; dense water formation; bioluminescence; optical photo-multiplier observationsFísica nuclearAcoustic Doppler Current ProfilerBioluminescenceAstrophysics - Instrumentation and Methods for AstrophysicsANTARES neutrino telescopeGeology[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Acoustic ADCP observationsCIRCULATIONFOS: Physical sciencesAquatic ScienceLIGURIAN SEAZooplanktonZooplanktonTelescopeAcoustic Doppler current profilerOCEANOPTICAL PHOTO-MULTIPLIERMediterranean Sea14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesLight reflectionANTARESAcoustic wave010505 oceanographyAdvectionDense waterElementary particlesZOOPLANKTON BIOMASSDoppler effectMARINE RESEARCHESGeophysics (physics.geo-ph)Boundary current[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Boundary currentsCONVECTION13. Climate actionFISICA APLICADAAdvectionEpisodic downward currentMediterranean Sea (Northwest)SYSTEMTelescopes
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The positioning system of the ANTARES Neutrino Telescope

2012

The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning sys…

Positioning systemDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Detector modelling and simulations II (electric fieldsDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesTiming detectorshardwareDetector alignment and calibration methods010303 astronomy & astrophysicsInstrumentationDETECTOR ALIGMENTMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSOUND[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Orientation (computer vision)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsTriangulation (computer vision)particle-beams)GeodesyDETECTOR CONTROL SYSTEMDetector modelling and simulations II (electric fields charge transport multiplication and induction pulse formation electron emission etc)Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)sources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pulse formationarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2DETECTOR MODELLING AND SIMULATIONSDetector modelling and simulations IIalgorithmsPhysics::Geophysics0103 physical sciences14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationetc)multiplication and inductionBuoyDetector control systems010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsMooringcharge transport[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Detector alignment and calibration methods (laserselectron emissionFISICA APLICADAdetector modelling and simulations ii (electric fields; antares neutrino telescope; multiplication and induction; charge transport; pulse formation; electron emission; etc); hardware; architecture; timing detectors; detector control systems (detector and experiment monitoring and slow-control systems; algorithms; databases); sources; detector alignment; calibration.; acoustic positioning; detector alignment and calibration methods (lasers; particle-beams)
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