6533b873fe1ef96bd12d56b1

RESEARCH PRODUCT

Performance of the First ANTARES Detector Line

C. ColnardRobert LahmannKouchner16 AntoineP. VerninJ. P. SchullerGregory David HallewellA. BigiA. BigiC. PicqF. LouisPiattelli27 PaoloJean-pierre ErnenweinH. LoehnerM. AnghinolfiM. AnghinolfiC. NaumannE. FalchiniE. FalchiniDominique LefèvreJ. BustoE. A. De WolfJ.-l. FudaM. CircellaM. RuppiG.e. Ip # V # La #G.e. Ip # V # La #G. WijnkerCorinne DonzaudP. PayreM. De JongF. DruilloleKay GrafJürgen BrunnerGuillaume LambardGuillaume LambardL. A. M. TascaPiera SapienzaM. BazzottiM. BazzottiGilles MaurinManuel Bou-caboFrancesco SimeoneFrancesco SimeoneTamburini ChristianHolger MotzA. RaduPh. CharvisG. Van Der SteenhovenJ. ZúñigaK. LyonsJ. Jeffrey CarrR. ConiglioneVincenzo CavasinniVincenzo CavasinniG. F. BurgioG. F. BurgioM. AgeronE. CastorinaE. CastorinaM. ArdidS. BasaR. BruijnYann HelloNasser Kalantar-nayestanakiJ. PetrovicG. CarminatiG. CarminatiG. GiacomelliG. GiacomelliV. BertinN. CottiniCamarena14 FranciscoS. KuchC. M. ReedH. CostantiniH. CostantiniJuan A. AguilarF. IschoeckCiro BigongiariDoriane DrouhinR. AuerU. F. KatzF. SalesaAnnarita MargiottaAnnarita MargiottaC. PettaC. PettaAlexander KappesSimona ToscanoM. MelissasJulien LavalleEberl12 ThomasG. LimE. PresaniChiarusi18 TommasoTommaso ChiarusiC. KopperG. GuillardJuan José HernándezArnauld AlbertP.m. KooijmanP.m. KooijmanD. ZaborovV. FlaminioV. FlaminioG. De BonisG. De BonisS. ManganoV. PopaM. MorgantiM. MorgantiH. LaschinskyC. RichardtM. RujoiuStephanie EscoffierJ.d. ZornozaD. CastelG.v. RussoG.v. RussoT. PradierW. KretschmerR. OstaschG. LelaizantG. LelaizantPatrick LamareS. BiagiS. BiagiD. DornicS. AnvarYvonne BecheriniOleg KalekinEmilio MignecoAnne DeschampsAlain MazureF. AmeliF. AmeliF. LucarelliF. LucarelliD. Lo PrestiD. Lo PrestiF. FehrS. CecchiniS. CecchiniS. CecchiniS. LoucatosM. VecchiM. VecchiJ. J. AubertJ. J. AubertM. MarcelinT. MontaruliAnton12 GiselaR. PilletC. RaccaH. LeiprovostH. LeiprovostP. CoyleR. IshanidzeR. IshanidzeJulien AublinM.c. BouwhuisP. DecowskiK. FratiniK. FratiniA. CaponeA. CaponeSpurio18 MaurizioMaurizio SpurioIvan DekeyserJ.a. Martínez-moraL. Moscoso

subject

MODULEPhysics::Instrumentation and DetectorsFOS: Physical sciencesAstrophysics01 natural sciencesNuclear physicsNEUTRINO TELESCOPESAngular distributionantares; deep-sea; first line; neutrino0103 physical sciencesNeutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]WATERAngular resolutionNEUTRINO TELESCOPE010306 general physicsATMOSPHERIC MUONSAstroparticle physicsPhysicsMuonANTARES010308 nuclear & particles physicsAstrophysics (astro-ph)DetectorDeep-seaAstronomy and AstrophysicsTime resolutionGeodesyMUON FLUXFirst lineSINGLEFísica nuclearUNDERWATER DETECTORLine (text file)NeutrinoSYSTEM

description

In this paper we report on the data recorded with the first Antares detector line. The line was deployed on the 14th of February 2006 and was connected to the readout two weeks later. Environmental data for one and a half years of running are shown. Measurements of atmospheric muons from data taken from selected runs during the first six months of operation are presented. Performance figures in terms of time residuals and angular resolution are given. Finally the angular distribution of atmospheric muons is presented and from this the depth profile of the muon intensity is derived.

10.1016/j.astropartphys.2009.02.008http://hal.in2p3.fr/in2p3-00365372