6533b832fe1ef96bd129a41a
RESEARCH PRODUCT
The ANTARES telescope neutrino alert system
V. BertinG. HalladjianP. PayreF. M. SchoeckG. LimFrancisco CamarenaKay GrafD. ZaborovJos SteijgerC. BogazziZ. CharifJ.-p. ErnenweinMaurizio SpurioMaurizio SpurioThomas EberlC. DistefanoJürgen BrunnerA.j. HeijboerAnnarita MargiottaAnnarita MargiottaD. Lo PrestiD. Lo PrestiK. PayetSimona ToscanoC. RaccaG.e. PăvălaşN. Picot-clementeA. EnzenhoeferE. A. De WolfJuanan AguilarG. WijnkerMichel AndréG.v. RussoG.v. RussoA. SpiesManuel Bou-caboFrancesco SimeoneFrancesco SimeoneD. DornicHolger MotzI. KreykenbohmV. Van ElewyckM. TaiutiM. TaiutiM. CircellaPatrick LamareA. C.s. Assis JesusCiro BigongiariA. RostovtsevTri L. AstraatmadjaU. F. KatzS. GalatàJ. HartmanP.m. KooijmanP.m. KooijmanA. BigiGiuseppina LarosaA. Sánchez-losaC. CarloganuF. SalesaRezo ShanidzeOleg KalekinAntoine KouchnerThierry PradierThierry PradierVladimir KulikovskiyVladimir KulikovskiyM. ArdidMatthias KadlerM. P. DecowskiPiera SapienzaAthina MeliS. AnvarU. FritschPaolo FermaniPaolo FermaniA. CaponeA. CaponeTh. StolarczykA. AlbertC. C. HsuTeresa MontaruliTeresa MontaruliV. GiordanoG. VannoniK. RoenschY. HelloY. HelloManuela VecchiManuela VecchiH. Van HarenF. FolgerAnne DeschampsC. DonzaudC. DonzaudI. Al SamaraiChristian TamburiniChristian TamburiniAlexander KappesR. ConiglioneF. SchuesslerJ. CarrDominique LefèvreDominique LefèvrePaolo PiattelliB. BaretS. LoucatosJ. PetrovicG. GiacomelliG. GiacomelliB. VallageM. FerriH. YepesD. PalioselitisDoriane DrouhinO. KavatsyukC. RivièreV. FlaminioV. FlaminioH. LoehnerJp SchullerI. DekeyserI. DekeyserJose BustoRobert LahmannS. BasaJ. ZúñigaE. PresaniB. HeroldS. BiagiS. BiagiTommaso ChiarusiC. KopperGregory David HallewellB. BouhouM. MarcelinGisela AntonA. RobertV. PopaJ.-l. FudaJ.-l. FudaP. CoyleM. RujoiuStephanie EscoffierC. CurtilD. LattuadaJ-j. AubertC. ReedJ.d. ZornozaJ. HoesslG. GuillardC. RichardtR. RichterS. ManganoM. NeffHeide CostantiniHeide CostantiniM. AgeronJ.a. Martínez-moraJ. Ruiz-rivasU. EmanueleE. NezriM.c. BouwhuisJuan José Hernández-reyPh. CharvisPh. CharvisM. De JongG. CarminatiG. CarminatiJörn WilmsS. CecchiniJ. P. Gómez-gonzálezM. AnghinolfiQ. DorostiP. VerninL. Moscososubject
Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[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]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burstdescription
The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.
year | journal | country | edition | language |
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2012-03-01 |