6533b823fe1ef96bd127edb6

RESEARCH PRODUCT

Performance of the front-end electronics of the ANTARES neutrino telescope

E. DelagnesFrancisco CamarenaR. OstaschC. CarloganuD. Lo PrestiM. ArdidAnnarita MargiottaAnnarita MargiottaY. HelloAntoine KouchnerF. LucarelliF. LucarelliJ. J. AubertJ. J. AubertVincent BertinVincent BertinF. FehrJ. PoinsignonG.v. RussoOleg KalekinNasser Kalantar-nayestanakiG. VannoniM. CircellaM. MorgantiM. MorgantiE. CastorinaE. CastorinaJ.-p. ErnenweinJ.-p. ErnenweinGisela AntonT. LegouT. LegouC. PicqE. FalchiniE. FalchiniDominique LefèvreDominique LefèvreC. RichardtE. A. De WolfD. DornicD. DornicD. DornicJ. FopmaJ. PetrovicJuanan AguilarG. WijnkerU. EmanueleG. GiacomelliG. GiacomelliC. NaumannM. RujoiuStephanie EscoffierStephanie EscoffierM.c. BouwhuisW. KretschmerGiorgio RiccobenePaolo PiattelliF. RethoreF. RethoreG. HalladjianG. HalladjianCiro BigongiariH. LafouxU. F. KatzD. PalioselitisDoriane DrouhinJ.d. ZornozaJürgen BrunnerJürgen BrunnerA. Le Van SuuA. Le Van SuuK. FratiniK. FratiniV. Van ElewyckThierry PradierH. LoehnerTeresa MontaruliTeresa MontaruliJ. P. SchullerC. HoffmannG. GuillardCh OlivettoCh OlivettoCh OlivettoHolger MotzG. E. PavalaS. ManganoH. CostantiniC. M. ReedC. M. ReedManuel Bou-caboFrancesco SimeoneM. NeffF. M. SchoeckM. De JongR. AuerA. CaponeA. CaponeJ. HoesslAnne DeschampsAnne DeschampsAlain MazureP. PayreP. PayreB. BaretS. BasaAlexander KappesS. BiagiS. BiagiManuela VecchiG. CarminatiG. CarminatiH. YepesS. LoucatosH. Le ProvostL. TascaV. FlaminioV. Flaminio[No Value] Charvis[No Value] CharvisPatrick LamareA. C.s. Assis JesusG. LimP. VerninTri L. AstraatmadjaTh. StolarczykJ-p PineauJ.a. Martínez-moraTh. ChaleilN. CottiniU. FritschP.m. KooijmanP.m. KooijmanGuillaume LambardGuillaume LambardM. MarcelinRobert LahmannS. AnvarV. PopaH. Van HarenE. PresaniB. HeroldC. CurtilC. CurtilN. Chon SenF. FeinsteinF. FeinsteinA. BrownA. BrownTommaso ChiarusiI. DekeyserI. DekeyserC. KopperA. RaduJos SteijgerG. De BonisG. De BonisGiuseppina LarosaD. ZaborovChristian TamburiniChristian TamburiniJ.-l. FudaJ.-l. FudaJ. ZúñigaGregory David HallewellGregory David HallewellC. DonzaudC. DonzaudJ. P. Gómez-gonzálezD. LachartreVincenzo CavasinniVincenzo CavasinniC. DistefanoE. MonmartheL. CaponettoKay GrafB. VallageArnauld AlbertM. AnghinolfiJ. BustoJ. BustoPiera SapienzaM. BazzottiM. BazzottiThomas EberlL. MoscosoG. LelaizantG. LelaizantF. SalesaS. CecchiniS. CecchiniJ. CarrJ. CarrF. DruilloleN. De BottonH. LaschinskySimona ToscanoC. RaccaN. Picot-clementeN. Picot-clementeRezo ShanidzeP. CoyleP. CoyleMaurizio SpurioMaurizio SpurioA.j. HeijboerJuan José Hernández-reyI. Al SamaraiI. Al Samarai

subject

Nuclear and High Energy PhysicsPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsOptical linkDigital dataFOS: Physical sciencesAnalog-to-digital converterNeutrino telescope01 natural sciencesMultiplexinglaw.inventionPhototubeApplication-specific integrated circuitPhotomultiplier tubelawASICs0103 physical sciences14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationPhysics010308 nuclear & particles physicsbusiness.industryASICAstrophysics::Instrumentation and Methods for AstrophysicsElectrical engineeringCIRCUITFront-end electronicsChip[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Física nuclearUNDERWATER DETECTORasic; front-end electronics; neutrino telescope; photomultiplier tubeAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSYSTEM

description

ANTARES is a high-energy neutrino telescope installed in the Mediterranean Sea at a depth of 2475 m. It consists of a three-dimensional array of optical modules, each containing a large photomultiplier tube. A total of 2700 front-end ASICs named Analogue Ring Samplers (ARS) process the phototube signals, measure their arrival time, amplitude and shape as well as perform monitoring and calibration tasks. The ARS chip processes the analogue signals from the optical modules and converts information into digital data. All the information is transmitted to shore through further multiplexing electronics and an optical link. This paper describes the performance of the ARS chip; results from the functionality and characterization tests in the laboratory are summarized and the long-term performance in the apparatus is illustrated.

https://doi.org/10.1016/j.nima.2010.06.225