Search results for "Cherenkov"

showing 10 items of 142 documents

A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory

2020

The High Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) continuously detects TeV photons and particles within its large field-of-view, accumulating every day a deeper exposure of two thirds of the sky. We analyzed 1523~days of HAWC live data acquired over four and a half years, in a follow-up analysis of {138} nearby ($z<0.3$) active galactic nuclei from the {\em Fermi} 3FHL catalog culminating within $40^\circ$ of the zenith at Sierra Negra, the HAWC site. This search for persistent TeV emission used a maximum-likelihood analysis assuming intrinsic power-law spectra attenuated by pair production of gamma-ray photons with the extragalactic background light. HAWC clearly detects persi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleusRadio galaxymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaGamma rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsExtragalactic background lightSpace and Planetary ScienceObservatorySkyBlazarAstrophysics - High Energy Astrophysical PhenomenaCherenkov radiationmedia_common
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Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events

2021

We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA using the populations simulated by the FIRESONG software to resemble the diffuse astrophysical neutrino flux measured by IceCube. We derive the detection probability for different zenith angles and geomagnetic field configurations. The difference in detectability of sources between CTA-North and CTA-South for the average geomagnetic field is not substantial. We investigate the effect of a higher night-sky background and the preliminary CTA Alpha layout on the detection probability.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesFluxAstrophysicsCherenkov Telescope ArrayEarth's magnetic fieldTarget of opportunitySensitivity (control systems)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaZenithAstrophysics - Cosmology and Nongalactic Astrophysics
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Rapidity correlations in Lambda baryon and proton production in hadronic Z0 decays

1998

In an analysis of multihadronic events recorded at LEP by DELPHI in the years 1992 through 1994, charged hadrons are identified using the measurement of their energy loss and their Cherenkov angle. Rapidity correlations of \La-\La, proton-proton, and \La-proton pairs are compared. The agreement with the string and cluster fragmentation models is tested. For those pairs that frame a meson in terms of rapidity the compensation of strangeness is studied. For \La{}$\overline{\mathrm{p}}$ pairs the additional correlation with respect to charged kaons is analysed.

IMAGING CHERENKOV DETECTOR; DELPHIParticle physicsNuclear and High Energy PhysicsMesonElectron–positron annihilationHadronNuclear TheoryStrangenessLambdaLambda baryon01 natural sciencesPartícules (Física nuclear)Nuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Rapidity010306 general physicsNuclear ExperimentDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERIMAGING CHERENKOV DETECTORLarge Electron–Positron ColliderPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentParticle Physics - Experiment
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Synthesis and study of new fluorescent probes for optical imaging, Cherenkov imaging and multimodal imaging

2015

The goal of this work was to prepare and study new fluorescent probes, which could give rise to novel optical or Cherenkov imaging agents. The first section of this work describes the synthesis of fluorescent subphthalocyanines and phthalocyanines probes, which possess relevant chemicals groups suitable for optical imaging applications. The optical and physico-chemical properties of the new probes were carefully examined to ensure they comply with the specification of the fluorophores for the desired application. The second part focused on the subsequent development of a few selected probes into real imaging agents. The biovectorisation of subphtalocyanines was achieved upon conjugation of …

Imagerie CherenkovPhthalocyaninesOptical ImagingCherenkov ImagingSubphthalocyaninesTitania nanotubesMultimodal ImagingUSPIO[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistryLiposomePhtalocyanines[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistryDOTAImagerie optiqueImagerie multimodaleNanotubes d’oxyde de titaneFluorescéineSubphtalocyaninesFluoresceine
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An anomaly in inclusive pion double charge exchange on 16O at about 1GeV

1996

The new results on the inclusive double charge exchange (DCX) reaction 16O(π-,π+)X at incident kinetic energy T0=0.75 and 1.15GeV are presented. The data were taken without using Cherentov counters. The new DCX cross sections agree well with the old ones. Both the values are about an order of magnitude larger than the theoretical cross sections calculated for the standard sequential mechanism. Two other approaches wich seem to explain the discrepancy are also briefly reviewed. Vicente Vacas, Manuel Jose, Manuel.J.Vicente@ific.uv.es

Inclusive double charge exchangeUNESCO::FÍSICA::Nucleónica:FÍSICA [UNESCO]Cherenkov countersUNESCO::FÍSICAInclusive double charge exchange ; Cherenkov counters ; Standard sequencial mechanismStandard sequencial mechanism:FÍSICA::Nucleónica [UNESCO]
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The THESEUS space mission concept: science case, design and expected performances

2018

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing …

IonizationAtmospheric Sciencecosmological modelCherenkov Telescope Array[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyDark ageMASSIVE SINGLE STARSStar formation rates Gamma ray01 natural sciencesCosmology: observationlocalizationlaw.inventionAstrophysicEinstein Telescopeobservational cosmologylawObservational cosmologyRe-ionizationCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionizationLIGOobservations [Cosmology]Telescope010303 astronomy & astrophysicsHigh sensitivityHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMulti-wavelengthenergy: highsezelegamma-ray burstsCosmology: observationsCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionization; Aerospace Engineering; Space and Planetary ScienceAstrophysics::Instrumentation and Methods for Astrophysicsimagingstar: formationburst [Gamma-ray]observatoryGeophysicsDark agesX rays Cosmology: observationAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenasignatureStarTIDAL DISRUPTIONGamma-ray: burstAstrophysics::High Energy Astrophysical PhenomenaSIMILAR-TO 6Socio-culturaleFOS: Physical sciencesAerospace EngineeringGamma-ray: burstsobservation [Cosmology]galaxy: luminosityX-ray astronomy: instrumentation7 CANDIDATE GALAXIESAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burst114 Physical sciencesSettore FIS/03 - Fisica della MateriaTelescopeX-raybursts [Gamma-ray]FIS/05 - ASTRONOMIA E ASTROFISICASettore FIS/05 - Astronomia e AstrofisicaFirst star0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]KAGRAInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsFirst starsLIGHT CURVESEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and Astrophysics115 Astronomy Space scienceCherenkov Telescope ArrayredshiftsensitivityRedshiftNEUTRON-STAR MERGERmessengerVIRGOelectromagneticLUMINOSITY FUNCTIONSpace and Planetary ScienceBLACK-HOLEGeneral Earth and Planetary SciencesGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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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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Cosmic ray composition and energy spectrum from 1–30 PeV using the 40-string configuration of IceTop and IceCube

2012

Astroparticle physics 42, 15 - 32 (2013). doi:10.1016/j.astropartphys.2012.11.003

Knee regionAstrophysicsTracking (particle physics)01 natural sciencesParticle identificationIceCubeTRACKINGWATERCherenkovNeutrino energyNEUTRINO TELESCOPEUltra-high-energy cosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSEADetectorAstrophysics::Instrumentation and Methods for AstrophysicsLIGHTComposition; Cosmic rays; Energy spectrum; IceCube; IceTop; Knee regionddc:540IceTopPARTICLE IDENTIFICATIONAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsIceCube detectorCompositionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2IceCube Neutrino ObservatorySEARCHESAccelerationcosmic raysdE/dx0103 physical sciences010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationTruncated meanMuon energy010308 nuclear & particles physicsAstronomyAstronomy and Astrophysics540Physics and AstronomycompositionEnergy SpectrumTEVEnergy spectrum
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Dual Cherenkov Radiation-Induced Near-Infrared Luminescence Imaging and Photodynamic Therapy toward Tumor Resection

2020

International audience; Cherenkov radiation (CR), the blue light seen in nuclear reactors, is emitted by some radiopharmaceuticals. This study showed that (1) a portion of CR could be transferred in the region of the optical spectrum, where biological tissues are most transparent: as a result, upon radiance amplification in the near-infrared window, the detection of light could occur twice deeper in tissues than during classical Cherenkov luminescence imaging and (2) Cherenkov-photodynamic therapy (CR-PDT) on cells could be achieved under conditions mimicking unlimited depth using the CR-embarked light source, which is unlike standard PDT, where light penetration depth is limited in biologi…

LuminescenceLightInfrared RaysInfraredPhthalocyaninesmedicine.medical_treatmentBodipyPhotodynamic therapy01 natural sciencesEnergy-transferMice03 medical and health sciencesOpticsUnresectedCell Line TumorQuantum DotsDrug DiscoverymedicineAnimalsCherenkov radiation030304 developmental biology0303 health sciencesChemistrybusiness.industryOptical ImagingCerenkov Radiation[SDV.SP]Life Sciences [q-bio]/Pharmaceutical sciences0104 chemical sciencesRecognition010404 medicinal & biomolecular chemistryPhotochemotherapyBright EnoughRadianceNanoparticlesMolecular MedicineAntenna (radio)Reactive Oxygen SpeciesLuminescencebusinessVisible spectrumJournal of Medicinal Chemistry
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Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays

2014

We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation $\gamma$-rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to $3.01 \times 10^{20}$ protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the $4-30$ MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background …

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and DetectorsC-12FOS: Physical sciencesAstronomy & Astrophysicslaw.inventionHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsSUPER-KAMIOKANDE DETECTORCross section (physics)High Energy Physics - Experiment (hep-ex)lawEXCITATIONABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGO-16Nuclear ExperimentPhysicsCALIBRATIONScience & TechnologyNeutral currenthep-exPhysicsGamma rayT2K experimentFísica3. Good healthPhysical SciencesNeutrinoWEAKFiducial markerBeam (structure)
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