Studying bioluminescence flashes with the ANTARES deep-sea neutrino telescope

IF 2.1 3区 地球科学 Q2 LIMNOLOGY
Nico Reeb, Sebastian Hutschenreuter, Philipp Zehetner, Torsten Ensslin, A. Albert, S. Alves, M. André, M. Anghinolfi, G. Anton, M. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa, B. Belhorma, M. Bendahman, V. Bertin, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M. C. Bouwhuis, H. Brânzaş, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, A. Capone, L. Caramete, J. Carr, V. Carretero, S. Celli, M. Chabab, T. N. Chau, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, A. Coleiro, M. Colomer-Molla, R. Coniglione, P. Coyle, A. Creusot, A. F. Díaz, G. de Wasseige, A. Deschamps, C. Distefano, I. Di Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, T. van Eeden, N. El Khayati, A. Enzenhöfer, P. Fermani, G. Ferrara, F. Filippini, L. Fusco, Y. Gatelet, P. Gay, H. Glotin, R. Gozzini, R. Gracia Ruiz, K. Graf, C. Guidi, S. Hallmann, H. van Haren, A. J. Heijboer, Y. Hello, J. J. Hernández-Rey, J. Hößl, J. Hofestädt, F. Huang, G. Illuminati, C. W. James, B. Jisse-Jung, M. de Jong, P. de Jong, M. Jongen, M. Kadler, O. Kalekin, U. Katz, N. R. Khan-Chowdhury, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, R. Le Breton, D. Lefèvre, E. Leonora, G. Levi, M. Lincetto, D. Lopez-Coto, S. Loucatos, L. Maderer, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J. A. Martínez-Mora, K. Melis, P. Migliozzi, A. Moussa, R. Muller, L. Nauta, S. Navas, E. Nezri, B. Ó Fearraigh, M. Organokov, G. E. Păvălaş, C. Pellegrino, M. Perrin-Terrin, P. Piattelli, C. Pieterse, C. Poirè, V. Popa, T. Pradier, N. Randazzo, S. Reck, G. Riccobene, A. Romanov, A. Sánchez-Losa, F. Salesa Greus, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, J. Schumann, F. Schüssler, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, S.J. Tingay, B. Vallage, V. Van Elewyck, F. Versari, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli, A. Zegarelli, J. D. Zornoza, J. Zúñiga, (ANTARES Collaboration)
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Drouhin,&nbsp;T. Eberl,&nbsp;T. van Eeden,&nbsp;N. El Khayati,&nbsp;A. Enzenhöfer,&nbsp;P. Fermani,&nbsp;G. Ferrara,&nbsp;F. Filippini,&nbsp;L. Fusco,&nbsp;Y. Gatelet,&nbsp;P. Gay,&nbsp;H. Glotin,&nbsp;R. Gozzini,&nbsp;R. Gracia Ruiz,&nbsp;K. Graf,&nbsp;C. Guidi,&nbsp;S. Hallmann,&nbsp;H. van Haren,&nbsp;A. J. Heijboer,&nbsp;Y. Hello,&nbsp;J. J. Hernández-Rey,&nbsp;J. Hößl,&nbsp;J. Hofestädt,&nbsp;F. Huang,&nbsp;G. Illuminati,&nbsp;C. W. James,&nbsp;B. Jisse-Jung,&nbsp;M. de Jong,&nbsp;P. de Jong,&nbsp;M. Jongen,&nbsp;M. Kadler,&nbsp;O. Kalekin,&nbsp;U. Katz,&nbsp;N. R. Khan-Chowdhury,&nbsp;A. Kouchner,&nbsp;I. Kreykenbohm,&nbsp;V. Kulikovskiy,&nbsp;R. Lahmann,&nbsp;R. Le Breton,&nbsp;D. Lefèvre,&nbsp;E. Leonora,&nbsp;G. Levi,&nbsp;M. Lincetto,&nbsp;D. Lopez-Coto,&nbsp;S. Loucatos,&nbsp;L. Maderer,&nbsp;J. Manczak,&nbsp;M. Marcelin,&nbsp;A. Margiotta,&nbsp;A. Marinelli,&nbsp;J. A. Martínez-Mora,&nbsp;K. Melis,&nbsp;P. Migliozzi,&nbsp;A. Moussa,&nbsp;R. Muller,&nbsp;L. Nauta,&nbsp;S. 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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. 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引用次数: 1

Abstract

We 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.

Abstract Image

用ANTARES深海中微子望远镜研究生物发光
我们开发了一种新的技术,利用水下中微子望远镜提供的大量数据集来获取深海生物发光的信息。望远镜的被动特性给了我们一个独特的机会来推断生物发光生物的信息,而不主动干扰它们。我们提出了一种统计方法,使我们能够重建单个生物体的发光,以及它们的位置和运动。建立了水下中微子望远镜测量过程和生物信号产生的数学模型。采用度量高斯变分推理算法,利用光电倍增管记录的光子计数重建模型参数。我们将该方法应用于合成数据集和ANTARES中微子望远镜收集的数据。该望远镜位于法国海岸40公里外,固定在海底2475米深的地方。合成数据的运行表明,我们可以模拟生物体发出的生物发光闪光。此外,我们发现光源定位的空间分辨率在很大程度上取决于望远镜的配置。精确测量探测器的效率和水的衰减长度对于重建光发射至关重要。最后,应用于ANTARES数据揭示了首次使用中微子望远镜数据定位生物发光生物。
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来源期刊
CiteScore
4.80
自引率
3.70%
发文量
56
审稿时长
3 months
期刊介绍: Limnology and Oceanography: Methods (ISSN 1541-5856) is a companion to ASLO''s top-rated journal Limnology and Oceanography, and articles are held to the same high standards. In order to provide the most rapid publication consistent with high standards, Limnology and Oceanography: Methods appears in electronic format only, and the entire submission and review system is online. Articles are posted as soon as they are accepted and formatted for publication. Limnology and Oceanography: Methods will consider manuscripts whose primary focus is methodological, and that deal with problems in the aquatic sciences. Manuscripts may present new measurement equipment, techniques for analyzing observations or samples, methods for understanding and interpreting information, analyses of metadata to examine the effectiveness of approaches, invited and contributed reviews and syntheses, and techniques for communicating and teaching in the aquatic sciences.
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