Studying bioluminescence flashes with the ANTARES deep‐sea neutrino telescope

Author:

Reeb Nico12ORCID,Hutschenreuter Sebastian13,Zehetner Philipp145,Ensslin Torsten14,Albert A.67,Alves S.8,André M.9,Anghinolfi M.10,Anton G.11,Ardid M.12,Aubert J.‐J.13,Aublin J.14,Baret B.14,Basa S.15,Belhorma B.16,Bendahman M.1417,Bertin V.13,Biagi S.18,Bissinger M.11,Boumaaza J.17,Bouta M.19,Bouwhuis M. C.20,Brânzaş H.21,Bruijn R.2022,Brunner J.13,Busto J.13,Caiffi B.10,Capone A.2324,Caramete L.21,Carr J.13,Carretero V.8,Celli S.2324,Chabab M.25,Chau T. N.14,El Moursli R. Cherkaoui17,Chiarusi T.26,Circella M.27,Coleiro A.14,Colomer‐Molla M.814,Coniglione R.18,Coyle P.13,Creusot A.14,Díaz A. F.28,de Wasseige G.14,Deschamps A.29,Distefano C.18,Di Palma I.2324,Domi A.1030,Donzaud C.1431,Dornic D.13,Drouhin D.67,Eberl T.11,van Eeden T.20,El Khayati N.17,Enzenhöfer A.13,Fermani P.2324,Ferrara G.18,Filippini F.2632,Fusco L.13,Gatelet Y.14,Gay P.1433,Glotin H.34,Gozzini R.11,Gracia Ruiz R.20,Graf K.11,Guidi C.1030,Hallmann S.11,van Haren H.35,Heijboer A. J.20,Hello Y.29,Hernández‐Rey J. J.8,Hößl J.11,Hofestädt J.11,Huang F.6,Illuminati G.142632,James C. W.36,Jisse‐Jung B.20,de Jong M.2037,de Jong P.20,Jongen M.20,Kadler M.38,Kalekin O.11,Katz U.11,Khan‐Chowdhury N. R.8,Kouchner A.14,Kreykenbohm I.39,Kulikovskiy V.10,Lahmann R.11,Le Breton R.14,Lefèvre D.4041,Leonora E.42,Levi G.2632,Lincetto M.13,Lopez‐Coto D.43,Loucatos S.1444,Maderer L.14,Manczak J.8,Marcelin M.15,Margiotta A.2632,Marinelli A.45,Martínez‐Mora J. A.12,Melis K.2022,Migliozzi P.45,Moussa A.19,Muller R.20,Nauta L.20,Navas S.43,Nezri E.15,Fearraigh B. Ó20,Organokov M.6,Păvălaş G. E.21,Pellegrino C.264647,Perrin‐Terrin M.13,Piattelli P.18,Pieterse C.8,Poirè C.12,Popa V.21,Pradier T.6,Randazzo N.42,Reck S.11,Riccobene G.18,Romanov A.1030,Sánchez‐Losa A.827,Salesa Greus F.8,Samtleben D. F. E.2037,Sanguineti M.1030,Sapienza P.18,Schnabel J.11,Schumann J.11,Schüssler F.44,Spurio M.2632,Stolarczyk Th.44,Taiuti M.1030,Tayalati Y.17,Tingay S.J.36,Vallage B.1444,Van Elewyck V.1448,Versari F.142632,Viola S.18,Vivolo D.4549,Wilms J.39,Zavatarelli S.10,Zegarelli A.2324,Zornoza J. D.8,Zúñiga J.8,

Affiliation:

1. Information Field Theory Group Max Planck Institute for Astrophysics Garching Germany

2. TUM School of Computation, Information and Technology Technical University of Munich Garching Germany

3. Department of Astrophysics/IMAPP Radboud University Nijmegen Nijmegen The Netherlands

4. Department of Physics, Ludwig‐Maximilians University Munich Germany

5. CERN Geneva Switzerland

6. Université de Strasbourg, CNRS, IPHC UMR 7178 Strasbourg France

7. Université de Haute Alsace Mulhouse France

8. IFIC—Instituto de Física Corpuscular (CSIC—Universitat de València) Paterna Valencia Spain

9. Technical University of Catalonia, Laboratory of Applied Bioacoustics Barcelona Spain

10. INFN—Sezione di Genova Genova Italy

11. Friedrich‐Alexander‐Universität Erlangen‐Nürnberg, Erlangen Centre for Astroparticle Physics Erlangen Germany

12. Institut d'Investigació per a la Gestió Integrada de les Zones Costaneres (IGIC)—Universitat Politècnica de València Gandia Spain

13. Aix Marseille Univ., CNRS/IN2P3, CPPM Marseille France

14. Université de Paris, CNRS, Astroparticule et Cosmologie Paris France

15. Aix Marseille Univ, CNRS, CNES, LAM Marseille France

16. National Center for Energy Sciences and Nuclear Techniques Rabat Morocco

17. Faculty of Sciences University Mohammed V in Rabat Rabat Morocco

18. INFN—Laboratori Nazionali del Sud (LNS) Catania Italy

19. Laboratory of Physics of Matter and Radiations University Mohammed I Oujda Morocco

20. Nikhef, Science Park Amsterdam The Netherlands

21. Institute of Space Science Măgurele Romania

22. Universiteit van Amsterdam, Instituut voor Hoge‐Energie Fysica Amsterdam The Netherlands

23. INFN—Sezione di Roma Roma Italy

24. Dipartimento di Fisica Università La Sapienza Roma Italy

25. LPHEA, Faculty of Science—Semlali Cadi Ayyad University Marrakech Morocco

26. INFN—Sezione di Bologna Bologna Italy

27. INFN—Sezione di Bari Bari Italy

28. Department of Computer Architecture and Technology/CITIC University of Granada Granada Spain

29. Géoazur, UCA, CNRS, IRD, Observatoire de la Côte d'Azur Sophia Antipolis France

30. Dipartimento di Fisica dell'Università Genova Italy

31. Université Paris‐Sud Orsay Cedex France

32. Dipartimento di Fisica e Astronomia dell'Università Bologna Italy

33. Laboratoire de Physique Corpusculaire, Clermont Université, Université Blaise Pascal, CNRS/IN2P3 Clermont‐Ferrand France

34. LIS, UMR Université de Toulon, Aix Marseille Université, CNRS Toulon France

35. Royal Netherlands Institute for Sea Research (NIOZ) Texel The Netherlands

36. International Centre for Radio Astronomy Research, Curtin University Bentley Western Australia Australia

37. Huygens‐Kamerlingh Onnes Laboratorium, Universiteit Leiden Leiden The Netherlands

38. Institut für Theoretische Physik und Astrophysik, Universität Würzburg Würzburg Germany

39. Dr. Remeis‐Sternwarte and ECAP, Friedrich‐Alexander‐Universität Erlangen‐Nürnberg Bamberg Germany

40. Mediterranean Institute of Oceanography (MIO), Aix‐Marseille University Marseille Cedex 9 France

41. Université du Sud Toulon‐Var, CNRS‐INSU/IRD UM 110 La Garde Cedex France

42. INFN—Sezione di Catania Catania Italy

43. Departamento de Física Teórica y del Cosmos and C.A.F.P.E University of Granada Granada Spain

44. IRFU, CEA Université Paris‐Saclay Gif‐sur‐Yvette France

45. INFN—Sezione di Napoli Napoli Italy

46. Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi Rome Italy

47. INFN, CNAF Bologna Italy

48. Institut Universitaire de France Paris France

49. Dipartimento di Fisica dell'Università Federico II di Napoli Napoli Italy

Abstract

AbstractWe develop a novel technique to exploit the extensive data sets provided by underwater neutrino telescopes to gain information on bioluminescence in the deep sea. The passive nature of the telescopes gives us the unique opportunity to infer information on bioluminescent organisms without actively interfering with them. We propose a statistical method that allows us to reconstruct the light emission of individual organisms, as well as their location and movement. A mathematical model is built to describe the measurement process of underwater neutrino telescopes and the signal generation of the biological organisms. The Metric Gaussian Variational Inference algorithm is used to reconstruct the model parameters using photon counts recorded by photomultiplier tubes. We apply this method to synthetic data sets and data collected by the ANTARES neutrino telescope. The telescope is located 40 km off the French coast and fixed to the sea floor at a depth of 2475 m. The runs with synthetic data reveal that we can model the emitted bioluminescent flashes of the organisms. Furthermore, we find that the spatial resolution of the localization of light sources highly depends on the configuration of the telescope. Precise measurements of the efficiencies of the detectors and the attenuation length of the water are crucial to reconstruct the light emission. Finally, the application to ANTARES data reveals the first localizations of bioluminescent organisms using neutrino telescope data.

Funder

H2020 European Research Council

Centre National de la Recherche Scientifique

French Alternative Energies and Atomic Energy Commission

Commission européenne Office Européen de Lutte Antifraude

Institut Universitaire de France

Labex UnivEarthS

Alsace Regional Council

Conseil Régional Provence-Alpes-Côte d'Azur

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Junta de Andalucía

French Research Institute for Exploitation of the Sea

American Institute of Mathematics

Publisher

Wiley

Subject

Ocean Engineering

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