0000000001251728

AUTHOR

F. Simeone

showing 12 related works from this author

A fast algorithm for muon track reconstruction and its application to the ANTARES neutrino telescope.

2011

An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained …

Optical telescopesAMANDASelection proceduresRobust reconstructionMonte Carlo methodAtmospheric muonsReal-time applicationNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentFast algorithmsHigh Energy Physics - Experiment (hep-ex)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsDetectorMonte Carlo SimulationMonte Carlo methodsComputer simulationLIGHTddc:540Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAlgorithmAlgorithmsFLUXOnline monitoring[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciencesTrack reconstructionOptical telescopeNuclear physicsMuon tracks0103 physical sciencesAngular resolutionLight sources010306 general physicsOptical follow-upDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARESneutrino telescope; track reconstruction010308 nuclear & particles physicsCharged particlesTrack (disk drive)track reconstructionAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics - Data Analysis Statistics and ProbabilityFISICA APLICADAATMOSPHERIC NEUTRINOSNeutrino telescopesSYSTEMData Analysis Statistics and Probability (physics.data-an)
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Search for Cosmic Neutrino Point Sources with Four Year Data of the ANTARES Telescope

2012

In this paper, a time-integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an E ¿2 n; spectrum, these flux limits are at 1-10 ¿10¿8 GeV cm¿2 s¿1 for declinations ranging from ¿90° to 40°. Limits for specific models of RX J1713.7¿3946 and Vela X, which include information on the source morphology and spectrum, are also given.

cosmic neutrinosUNIVERSEFluxVela01 natural scienceslaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawSIGNALSABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]MAXIMUM-LIKELIHOOD010303 astronomy & astrophysicsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer database[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ASTRONOMYneutrinosastroparticle physicsFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaREMNANT RX J1713.7-3946Particle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescope[SDU.STU]Sciences of the Universe [physics]/Earth SciencesFOS: Physical sciencesddc:500.2Telescopeneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesPoint (geometry)ALGORITHMNeutrinosDETECTORCosmic raysUNDERWATER CHERENKOV NEUTRINO TELESCOPES010308 nuclear & particles physicsAstronomy and AstrophysicsHIGH-ENERGY PHOTONSSpace and Planetary ScienceFISICA APLICADAAstroparticle physics
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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Deep sea tests of a prototype of the KM3NeT digital optical module

2014

SIRE(opens in a new window)|View at Publisher| Export | Download | Add to List | More... European Physical Journal C Volume 74, Issue 9, 1 September 2014, 8p Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration (Article) Adrián-Martínez, S.a, Ageron, M.b, Aharonian, F.c, Aiello, S.d, Albert, A.e, Ameli, F.f, Anassontzis, E.G.g, Anghinolfi, M.h, Anton, G.i, Anvar, S.j, Ardid, M.a, de Asmundis, R.k, Balasi, K.l, Band, H.m, Barbarino, G.kn, Barbarito, E.o, Barbato, F.kn, Baret, B.p, Baron, S.p, Belias, A.lq, Berbee, E.m, van den Berg, A.M.r, Berkien, A.m, Bertin, V.b, Beurthey, S.b, van Beveren, V.m, Beverini, N.st, Biagi, S.uv, Bianucci, S.t, Billault, M.b,…

KM3NeT; digital optical modulePhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)TELESCOPEPhysics::Instrumentation and Detectorsdigital optical moduleFOS: Physical sciencesNeutrino Telescopesneutrino astrophysics; Cherenkov detector; Neutrino TelescopesKM3NeT; Cherenkov; UnderwaterDESIGNCherenkov[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)KM3NeTEngineering (miscellaneous)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeDATA-ACQUISITIONInstrumentation and Detectors (physics.ins-det)READOUTneutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]NEUTRINOSUnderwaterAstrophysics - Instrumentation and Methods for AstrophysicsSYSTEMCherenkov detector
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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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Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data

2013

Aims. We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Methods. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. Results. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to …

Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeMonte Carlo methodgamma-ray burst: generalFOS: Physical sciencesddc:500.201 natural sciencesCoincidenceSpectral lineGamma ray burstsmethods: numericalNuclear physicsneutrinoHigh Energy Physics - Phenomenology (hep-ph)Raigs gamma0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutrinsNeutrinos010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics:Desenvolupament humà i sostenible [Àrees temàtiques de la UPC]Muonnumerical [Methods]010308 nuclear & particles physicsneutrinosAstronomy and Astrophysicsgeneral [Gamma-ray burst]neutrinos - gamma-ray burst: general - methods: numerical; methods: numerical; neutrinos; gamma-ray burst: generalHigh Energy Physics - PhenomenologyGamma-ray burst: general; Methods: numerical; NeutrinosNeutrino detectorSpace and Planetary ScienceFISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoneutrinos - gamma-ray burst: general - methods: numericalGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration

2014

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deep waters of the Mediterranean Sea. This digital optical module has a novel design with a very large photocathode area segmented by the use of 31 three inch photomultiplier tubes. It has been integrated in the ANTARES detector for in-situ testing and validation. This paper reports on the first months of data taking and rate measurements. The analysis results highlight the capabilities of the new module design in terms of background suppression and signal recognition. The directionality of the optical module enables the recognition of multiple Cherenkov photons from the same $^{40…

PhysicsPhotomultiplierPhotonPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsbusiness.industryPhysics::Instrumentation and DetectorsDetectorAstrophysics::Instrumentation and Methods for Astrophysics01 natural sciencesSignalPhotocathodeOpticsKM3NeT0103 physical sciences14. Life underwaterSensitivity (control systems)010306 general physicsbusinessEngineering (miscellaneous); Physics and Astronomy (miscellaneous)Engineering (miscellaneous)Cherenkov radiation
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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Carbon monoxide improves cardiac energetics and safeguards the heart during reperfusion after cardiopulmonary bypass in pigs

2004

Ischemia-reperfusion injury, a clinical problem during cardiac surgery, involves worsened adenosine trisphosphate (ATP) generation and damage to the heart. We studied carbon monoxide ( CO) pretreatment, proven valuable in rodents but not previously tested in large animals, for its effects on pig hearts subjected to cardiopulmonary bypass with cardioplegic arrest. Hearts of CO-treated pigs showed significantly higher ATP and phosphocreatine levels, less interstitial edema, and apoptosis of cardiomyocytes and required fewer defibrillations after bypass. We conclude that treatment with CO improves the energy status, prevents edema formation and apoptosis, and facilitates recovery in a clinical…

Sus scrofaMyocardial IschemiaApoptosisCardiotonic AgentsBiochemistrylaw.inventionchemistry.chemical_compoundAdenosine Triphosphateischemia reperfusion; heart arrest; apoptosis; hypoxia; Adenosine Diphosphate; Adenosine Monophosphate; Adenosine Triphosphate; Animals; Apoptosis; Carbon Monoxide; Cardiotonic Agents; Edema; Electric Countershock; Energy Metabolism; Female; Guanosine Triphosphate; Heart; Myocardial Ischemia; Myocardial Reperfusion Injury; Myocytes Cardiac; NAD; NADP; Oxidation-Reduction; Sus scrofa; Cardiopulmonary BypasslawEdemaEdemaMyocytes CardiacCarbon MonoxideCardiopulmonary BypassMED/04 - PATOLOGIA GENERALEHeartCardiac surgeryAdenosine DiphosphateAnesthesiaCardiologyFemaleGuanosine Triphosphatemedicine.symptomCardiacOxidation-ReductionBiotechnologymedicine.drugischemia reperfusion; heart arrest; apoptosis; hypoxiaAdenosine monophosphatemedicine.medical_specialtyCardiotonic AgentsElectric CountershockMyocardial Reperfusion InjuryPhosphocreatineInternal medicineGeneticsmedicineCardiopulmonary bypassischemia reperfusionAnimalsMolecular BiologyMyocytesbusiness.industryhypoxiaNADAdenosineapoptosiAdenosine MonophosphateAdenosine diphosphatechemistryEnergy MetabolismbusinessNADPheart arrest
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Visual and Hearing Impairment Are Associated With Delirium in Hospitalized Patients: Results of a Multisite Prevalence Study

2021

Objective: Sensory deficits are important risk factors for delirium but have been investigated in single-center studies and single clinical settings. This multicenter study aims to evaluate the association between hearing and visual impairment or bi-sensory impairment (visual and hearing impairment) and delirium. Design: Cross-sectional study nested in the 2017 "Delirium Day" project. Setting and participants: Patients 65 years and older admitted to acute hospital medical wards, emergency departments, rehabilitation wards, nursing homes, and hospices in Italy. Methods: Delirium was assessed with the 4AT (a short tool for delirium assessment) and sensory deficits with a clinical evaluation. …

medicine.medical_specialtyActivities of daily livingCross-sectional studyHearing lossmedicine.medical_treatmentVisual impairmentPsychological interventionvisual impairmentSocio-culturalebehavioral disciplines and activitiesHearing impairment delirium older sensory deficits visual impairment.sensory deficitHearing impairment03 medical and health sciencesdelirium; Hearing impairment; older; sensory deficits; visual impairment0302 clinical medicinedeliriumRisk FactorsActivities of Daily Livingmental disordersmedicineolderHumansDementia030212 general & internal medicineLS4_4Hearing LossGeneral NursingRehabilitationbusiness.industryHealth PolicyGeneral Medicinemedicine.diseaseHearing impairment; delirium; older; sensory deficits; visual impairmentnervous system diseasesCross-Sectional StudiesItalyEmergency medicineDeliriumGeriatrics and Gerontologymedicine.symptomsensory deficitsbusiness030217 neurology & neurosurgerydelirium; Hearing impairment; older; sensory deficits; visual impairment; Activities of Daily Living; Cross-Sectional Studies; Humans; Italy; Risk Factors; Delirium; Hearing Loss
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Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

2013

Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric energy spectrum in the energy range 0.1-200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is similar to 25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)European Physical Journal C
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