4.4 Article

KM3NeT front-end and readout electronics system: hardware, firmware, and software

出版社

SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
DOI: 10.1117/1.JATIS.5.4.046001

关键词

front-end electronics; readout electronics; neutrino telescope; KM3NeT

资金

  1. Agence Nationale de la Recherche, France [ANR-15-CE31-0020]
  2. Centre National de la Recherche Scientifique (CNRS), France
  3. Commission Europeenne (FEDER fund), France
  4. Commission Europeenne (Marie Curie Program), France
  5. Institut Universitaire de France (IUF), France
  6. IdEx program, France
  7. UnivEarthS Labex program at Sorbonne Paris Cite, Paris Ile-de-France Region, France [ANR-10-LABX-0023, ANR-11-IDEX-0005-02]
  8. Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia [FR-18-1268]
  9. Deutsche Forschungsgemeinschaft (DFG), Germany
  10. General Secretariat of Research and Technology (GSRT), Greece
  11. Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), PRIN 2017 program Italy [NAT-NET 2017W4HA7S]
  12. Ministry of Higher Education, Scientific Research and Professional Training, Morocco
  13. Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands
  14. National Science Centre, Poland [2015/18/E/ST2/00758]
  15. National Authority for Scientific Research (ANCS), Romania
  16. Plan Estatal de Investigacion (MINECO/FEDER), Spain [FPA2015-65150-C3-1-P, FPA2015-65150-C3-2-P, FPA2015-65150-C3-3-P]
  17. Severo Ochoa Centre of Excellence program (MINECO), Spain
  18. Red Consolider MultiDark (MINECO), Spain [FPA2017-90566-REDC]
  19. Prometeo program (Generalitat Valenciana), Spain
  20. Grisolia program (Generalitat Valenciana), Spain
  21. la Caixa Foundation, Spain [100010434, LCF/BQ/IN17/11620019]
  22. European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant , Spain [713673]

向作者/读者索取更多资源

The KM3NeT research infrastructure being built at the bottom of the Mediterranean Sea will host water-Cherenkov telescopes for the detection of cosmic neutrinos. The neutrino telescopes will consist of large volume three-dimensional grids of optical modules to detect the Cherenkov light from charged particles produced by neutrino-induced interactions. Each optical module houses 31 3-in. photomultiplier tubes, instrumentation for calibration of the photomultiplier signal and positioning of the optical module, and all associated electronics boards. By design, the total electrical power consumption of an optical module has been capped at seven Watts. We present an overview of the front-end and readout electronics system inside the optical module, which has been designed for a 1-ns synchronization between the clocks of all optical modules in the grid during a life time of at least 20 years. (C) 2019 Society of Photo-Optical Instrumentation Engineers (SPIE)

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