0000000000100017

AUTHOR

D Zaborov

showing 2 related works from this author

Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and Ic…

2019

[EN] Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the out¿ow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCub…

Astrofísicacollapse [supernova]neutron star: binaryEVENTS GW150914Gravitació010504 meteorology & atmospheric sciencesneutrino: energy: highAstronomyRAYBinary numberbinary [neutron star]Astrophysics7. Clean energy01 natural sciencesPhysical ChemistryAtomicIceCubeneutrinoParticle and Plasma PhysicsAstronomi astrofysik och kosmologiblack holeAstronomy Astrophysics and CosmologyLIGO010303 astronomy & astrophysicsgravitational waveELECTROMAGNETIC SIGNALSQCQBSettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HE[PHYS]Physics [physics]Astrophysics::Instrumentation and Methods for Astrophysicsneutrinosgravitational waves; neutrinos520 Astronomie und zugeordnete Wissenschaftenddc:observatorySupernovagravitational wavesastrophysics: densityPhysical SciencesNeutrinoAstrophysics - High Energy Astrophysical Phenomenagravitational waves; neutrinos; Astronomy and Astrophysics; Space and Planetary ScienceAstronomical and Space SciencessignaturePhysical Chemistry (incl. Structural)supernova: collapseAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsGravitational wavesemission [gravitational radiation]Ones gravitacionalsCoincident0103 physical sciencesGravitational Waves Neutrinos LIGO Virgo Antares IceCubeNuclearddc:530Neutrinsenergy: high [neutrino]NeutrinosSTFCAstrophysiqueAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyANTARESGravitational waveVirgoOrganic ChemistryAstronomyRCUKMolecularAstronomy and AstrophysicsAstronomieAstronomy and Astrophysic530 PhysikLIGOSciences de l'espaceBlack holemessengerNeutron starAntaresPhysics and AstronomySpace and Planetary ScienceFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]gravitational radiation: emissiondensity [astrophysics]ddc:520[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]EMISSION
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Transmission of light in deep sea water at the site of the Antares neutrino telescope

2005

The ANTARES neutrino telescope is a large photomultiplier array designed to detect neutrino-induced upward-going muons by their Cherenkov radiation. Understanding the absorption and scattering of light in the deep Mediterranean is fundamental to optimising the design and performance of the detector. This paper presents measurements of blue and UV light transmission at the ANTARES site taken between 1997 and 2000. The derived values for the scattering length and the angular distribution of particulate scattering were found to be highly correlated, and results are therefore presented in terms of an absorption length lambda_abs and an effective scattering length lambda_sct^eff. The values for …

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsNeutrino telescopeAstrophysicsLambda01 natural sciencesLight scattering[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Sea water properties: absorption and transmission of lightHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAngular resolution07.89.+b 29.40.Ka 42.25.Bs 42.68.Xy 92.10.Bf 92.10.Pt 95.55.Vj010306 general physicsCherenkov radiationPhysicsneutrino telescope undersea Cherenkov detectors sea water properties absorption and transmission of lightUndersea Cherenkov detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsScatteringAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAttenuation lengthSea water properties: absorption and transmission of light.Astronomy and AstrophysicsScattering lengthabsorption and transmission of lightHigh Energy Physics - Phenomenology13. Climate actionFísica nuclearsea water propertiesAstroparticle Physics
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