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Exploring the sensitivity of next generation gravitational wavedetectors

Why is this work in the frame?

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

Canadian affiliationAn author listed a Canadian institution. This is the only route the usual frame has.

Classifier prediction

metacan-v1-d91a1de5be90

Predictions imitate two machine teachers. Scores are not calibrated prevalence probabilities.

Classifier candidate
ObservationalTheoretical or conceptual
Classifier consensus
Theoretical or conceptual
Teacher imitation scores

Codex

Theoretical or conceptual0.106
Observational0.050
Not applicable0.014
Bench or experimental0.010
Other design0.006
Bibliometrics0.000
Research integrity0.000
Systematic review0.000
Science and technology studies0.000
Metaresearch0.000
Case report0.000
Simulation or modelling0.000
Open science0.000
Qualitative0.000
Scholarly communication0.000
Meta-epidemiology (broad)0.000
Non-randomized trial0.000
Meta-analysis0.000
Meta-epidemiology (narrow)0.000
Randomized trial0.000

Gemma

Theoretical or conceptual0.240
Observational0.026
Not applicable0.005
Bench or experimental0.003
Simulation or modelling0.003
Qualitative0.001
Bibliometrics0.001
Metaresearch0.001
Research integrity0.000
Science and technology studies0.000
Meta-epidemiology (broad)0.000
Case report0.000
Scholarly communication0.000
Non-randomized trial0.000
Meta-epidemiology (narrow)0.000
Systematic review0.000
Open science0.000
Meta-analysis0.000
Randomized trial0.000

Machine scores (provisional)

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

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.

Opus teacher head0.155
GPT teacher head0.347
Teacher spread
0.192 how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Abstract

Abstract The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.

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.