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Record W3177827416 · doi:10.22323/1.395.1160

Optical analysis of the Pacific Ocean Neutrino Experiment (P-ONE) site using data from the first pathfinder mooring

2021· article· en· W3177827416 on OpenAlexaffabout
C. Fruck, Nicolai Bailly, Jeannette Bedard, M. Böhmer, Jeff Bosma, Dirk Brussow, Jonathan Cheng, K. Clark, Beckey Croteau, M. Danninger, Fabio De Leo, Nathan Deis, Matthew Ens, Rowan Fox, Andreas Gärtner, R. Gernhäuser, Darren Grant, Helen He, Felix Henningsen, K. Holzapfel, Ryan Hotte, Reyna Jenkyns, Hamish Johnson, Akanksha Katil, Claudio Kopper, C. B. Krauss, I. Kulin, K. Leismüller, Sally P. Leys, Tony T.Y. Lin, Paul Macoun, Thomas McElroy, S. Meighen-Berger, Jan Michel, R. W. Moore, Mike Morley, László Papp, B. Pirenne, Tom Qiu, Mark Rankin, I. C. Rea, E. Resconi, Adrian Round, Albert Ruskey, Ryan Rutley, Christian Spannfellner, Jakub Stacho, Ross Timmerman, Meghan Tomlin, Matt Tradewell, M. Traxler, Matt Uganecz, Seann Wagner, Juan Pablo Yáñez, Yinsong Zheng

Bibliographic record

VenueProceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021) · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsSimon Fraser UniversityUniversity of Alberta
Fundersnot available
KeywordsPathfinderNeutrinoMooringSoftware deploymentCherenkov radiationNeutrino detectorEnvironmental sciencePhysicsOceanographyGeologyComputer scienceNuclear physicsNeutrino oscillationOpticsWorld Wide WebDetector

Abstract

fetched live from OpenAlex

The Pacific Ocean Neutrino Experiment (P-ONE) is an initiative by a collaboration of Canadian and German universities as well as Ocean Networks Canada (ONC) to develop a new large-scale neutrino telescope 2600 m below the ocean off the coast of western Canada. While the instrumented volume needs to be at least on the order of km³ for the physics goals of P-ONE to be met, the density of photo sensors needs to be kept as low as possible in order to minimize construction costs. Naturally, this puts very high demands on the optical properties of water at the deployment site. Ideally, the water should exhibit minimal photon extinction and scattering to optimize the light yield and timing needed for reconstructing neutrino-induced Cherenkov light flashes. In addition, a low light background from natural undersea sources such as bioluminescence and K40 radioactive decay is necessary for achieving high sensitivity to neutrino events. In order to evaluate the proposed site for P-ONE, two pathfinder missions have been deployed successfully, one in 2018 and the other in 2020. We present the results from the first mission that was primarily aimed at evaluating the optical properties of the site in terms of attenuation length, and backgrounds.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.346
Threshold uncertainty score0.755

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.052
GPT teacher head0.269
Teacher spread0.216 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations5
Published2021
Admission routes2
Has abstractyes

Explore more

Same venueProceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)Same topicAstrophysics and Cosmic PhenomenaFrench-language works237,207