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Record W3179875204 · doi:10.22323/1.395.1197

Pacific Ocean Neutrino Experiment (P-ONE): prototype line development

2021· article· en· W3179875204 on OpenAlexaffabout
Christian Spannfellner, 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, C. Fruck, 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, 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 institutionsBurnaby HospitalQueen's UniversitySimon Fraser UniversityUniversity of Alberta
Fundersnot available
KeywordsPathfinderObservatoryLine (geometry)Remote sensingMeteorologyGeologyPhysicsComputer scienceAstronomy

Abstract

fetched live from OpenAlex

The Pacific Ocean Neutrino Experiment (P-ONE) is a new initiative to construct one of the world’s largest neutrino detectors in the deep Pacific Ocean off the coast of British Columbia, Canada. Located in the Cascadia Basin region, P-ONE builds on a number of key strengths within the Canadian oceanographic community. The Cascadia Basin monitoring site is part of the NEPTUNE observatory of Ocean Networks Canada (ONC), which provides power and data connections to various deep ocean sites, accessible to experiments. In cooperation with ONC, the collaboration successfully deployed two pathfinder experiments, the STRAW projects, in 2018 and 2020, respectively. These pathfinder mooring lines aim to measure the optical and ambient background characteristics of the Cascadia Basin in a depth of 2660m. The P-ONE prototype line is the successor of these mooring lines and the next step towards the P-ONE neutrino observatory. The main objective of the prototype line lies in the construction, deployment, and operation of a complete P-ONE mooring line as a proof of concept of the individual components. This line will comprise of P-ONE digital optical modules to measure the emerging Cherenkov radiation by neutrino-induced processes and P-ONE calibration devices to provide in-situ calibration of the detector. The prototype line will be complemented by external geometry calibration units to verify the envisioned calibration principles.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.007
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.002
Open science0.0030.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0070.005

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 head0.023
GPT teacher head0.250
Teacher spread0.227 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
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

Citations4
Published2021
Admission routes2
Has abstractyes

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