6533b7d5fe1ef96bd1265334

RESEARCH PRODUCT

First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

Antares CollaborationS. Adri��n-mart��nezJ. A. AguilarI. Al SamaraiA. AlbertM. Andr��M. AnghinolfiG. AntonS. AnvarM. ArdidA. C. Assis JesusT. AstraatmadjaJ-j. AubertB. BaretS. BasaV. BertinS. BiagiA. BigiC. BigongiariC. BogazziM. Bou-caboB. BouhouM. C. BouwhuisJ. BrunnerJ. BustoF. CamarenaA. CaponeC. CarloganuG. CarminatiJ. CarrS. CecchiniZ. CharifPh. CharvisT. ChiarusiM. CircellaR. ConiglioneH. CostantiniP. CoyleC. CurtilM. P. DecowskiI. DekeyserA. DeschampsC. DistefanoC. DonzaudD. DornicQ. DorostiD. DrouhinT. EberlU. EmanueleA. Enzenh��ferJ-p. ErnenweinS. EscoffierP. FermaniM. FerriV. FlaminioF. FolgerU. FritschJ-l. FudaS. Galat��P. GayG. GiacomelliV. GiordanoJ. P. G��mez-gonz��lezK. GrafG. GuillardG. HalladjianG. HallewellH. Van HarenJ. HartmanA. J. HeijboerY. HelloJ. J. Hern��ndez-reyB. HeroldJ. H����lC. C. HsuM. De JongM. KadlerO. KalekinA. KappesU. KatzO. KavatsyukP. KooijmanC. KopperA. KouchnerI. KreykenbohmV. KulikovskiyR. LahmannP. LamareG. LarosaD. LattuadaD. Lef��vreG. LimD. Lo PrestiH. LoehnerS. LoucatosS. ManganoM. MarcelinA. MargiottaJ. A. Mart��nez-moraA. MeliT. MontaruliL. MoscosoH. MotzM. NeffE. NezriD. PalioselitisG. E. PavalasK. PayetP. PayreJ. PetrovicP. PiattelliN. Picot-clementeV. PopaT. PradierE. PresaniC. RaccaC. ReedC. RichardtR. RichterC. Rivi��reA. RobertK. RoenschA. RostovtsevJ. Ruiz-rivasM. RujoiuG. V. RussoF. SalesaD. F. E. SamtlebenP. SapienzaF. Sch��ckJ-p. SchullerF. Sch��sslerT. SeitzR. ShanidzeF. SimeoneA. SpiesM. SpurioJ. J. M. SteijgerTh. StolarczykA. S��nchez-losaM. TaiutiC. TamburiniS. ToscanoB. VallageV. Van ElewyckG. VannoniM. VecchiP. VerninS. WagnerG. WijnkerJ. WilmsE. De WolfH. YepesD. ZaborovJ. D. ZornozaJ. Z����iga

subject

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

description

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.

10.13039/501100004837http://hdl.handle.net/10251/36278