First instrumented line of the Pacific Ocean Neutrino Experiment: status, development and outlook.

The Pacific Ocean Neutrino Experiment (P-ONE) is a planned water-based Cherenkov neutrino telescope that will be located off the west coast of Canada. P-ONE will observe high-energy astrophysical neutrinos, aiming to identify the sources where they are produced, and will allow long-term in-situ studies of bioluminescence in the Cascadia Basin. The detector will be composed of instrumented mooring lines, which, along with the existing deep-sea infrastructure of the NEPTUNE observatory, make the design easily scalable. The first phase of the experiment, called P-ONE-1, is the first complete detector line and is instrumented with 20 modules spanning one kilometer. P-ONE-1 will serve as a test for all the newly developed systems and infrastructure and will pave the way for the future phases. This contribution will give an overview of the current status of the construction of the first line, the expected performance and the recent design innovations.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.1087
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00

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article

First instrumented line of the Pacific Ocean Neutrino Experiment: status, development and outlook.

B. Biffard, C. Haack, V. Gousy-Leblanc, I. Taboada et al.
Astrophysics and Cosmic Phenomena
article

First instrumented line of the Pacific Ocean Neutrino Experiment: status, development and outlook.

B. Biffard, C. Haack, V. Gousy-Leblanc, I. Taboada, Kang Wang, László Papp, W. Noga, B. Pirenne, Lanfranco Muzi, C. Bellenghi, C. Kopper, Felix Henningsen, E. Price, Matthew Charlton, M. Heesemann, Pa. Malecki, Cristina Lagunas Gualda, Jeffrey Hutchinson, Shiv K. Sharma, M. Boehmer, D. Salazar-Gallegos, Christian Spannfellner, L. Ginzkey, B. Veenstra, A. Alexander Wight, R. Ørsøe, M. Danninger, C. Weaver, Jean Pierre Twagirayezu, R. W. Moore, Simeon Bash, Tobias Kerscher, Andrew J. Baron, Andreas Gärtner, M. Agostini, L. Schumacher, Shraddha Karanth, K. Kopański, M. Brandenburg, A. Scholz, P. Krause, K. Leismüller, Jakub Stacho, C. Miller, Franz Fuchs, N. Whitehorn, Torge Martin, A. Rahlin, P. Pfahler, D. Ghuman, L. Winter, P. S. Barbeau, C. B. Krauss, Adrian Ponce, R. C. Nichol, N. Kurahashi, B. Crudele, A. Zaalishvili, N. Cedarblade-Jones, Ruiqi Li, Juan Pablo Yáñez, T. DeYoung, M. U. Nisa, D. R. Grant, Victoria Alexis Parrish, S. Robertson, A. Grimes, G. Marshall, R. Halliday, E. Resconi, P. Bunton, J. Garriz, S. Agreda, T. Glukler, D. Hembroff, S. Loipolder, S. Magel, N. Molberg, B. Nührenbörger, M. Rangen, R. Wroński
article en

Abstract

The Pacific Ocean Neutrino Experiment (P-ONE) is a planned water-based Cherenkov neutrino telescope that will be located off the west coast of Canada. P-ONE will observe high-energy astrophysical neutrinos, aiming to identify the sources where they are produced, and will allow long-term in-situ studies of bioluminescence in the Cascadia Basin. The detector will be composed of instrumented mooring lines, which, along with the existing deep-sea infrastructure of the NEPTUNE observatory, make the design easily scalable. The first phase of the experiment, called P-ONE-1, is the first complete detector line and is instrumented with 20 modules spanning one kilometer. P-ONE-1 will serve as a test for all the newly developed systems and infrastructure and will pave the way for the future phases. This contribution will give an overview of the current status of the construction of the first line, the expected performance and the recent design innovations.

National Science Foundation, UK Research and Innovation, Deutsche Forschungsgemeinschaft, Canada First Research Excellence Fund, Alliance de recherche numérique du Canada, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council
Openalex Percentile: Top 89%
Astrophysics and Cosmic Phenomena
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