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Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

2016· article· en· 363 citations· W2277737850 on OpenAlex· 10.1088/0264-9381/33/13/134001

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.
Canadian funderA Canadian agency funded it. The work may carry no Canadian affiliation at all.

Full frame distilled prediction

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.

Candidate categories
none
Consensus categories
none
Domain
Candidate signal: noneConsensus signal: none
Study design
Candidate signal: Bench or experimentalConsensus signal: none
Genre
Candidate signal: EmpiricalConsensus signal: Empirical
Teacher disagreement score
0.832
Threshold uncertainty score
0.376
Validation status
machine_predicted_unvalidated · codex-gemma-dda1882f352a

Codex and Gemma teacher scores by category

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

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 head0.015
GPT teacher head0.290
Teacher spread
0.275 · 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

On September 14, 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.

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.

The record

Venue
Classical and Quantum Gravity
Topic
Pulsars and Gravitational Waves Research
Field
Physics and Astronomy
Canadian institutions
Canadian Institute for Theoretical AstrophysicsUniversity of Toronto
Funders
Division of Human Resource DevelopmentAustralian Research CouncilScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaMinistry of Science and Technology, TaiwanMinistry of Education, IndiaNarodowe Centrum NaukiNational Research Foundation of KoreaRoyal SocietyMinisterio de Economía y CompetitividadCouncil of Scientific and Industrial Research, IndiaCentre National de la Recherche ScientifiqueIndustry CanadaFundação de Amparo à Pesquisa do Estado de São PauloGovern de les Illes BalearsNederlandse Organisatie voor Wetenschappelijk OnderzoekEuropean CommissionRussian Foundation for Basic ResearchCanadian Institute for Advanced ResearchInstitut des Origines de LyonLeverhulme TrustScottish Funding CouncilScottish Universities Physics AllianceHungarian Scientific Research FundScience and Engineering Research BoardNational Science FoundationIstituto Nazionale di Fisica NucleareKavli FoundationResearch Corporation for Science Advancement
Keywords
LIGOPhysicsGravitational waveDetectorTransient (computer programming)Noise (video)SIGNAL (programming language)Binary black holeEvent (particle physics)AstrophysicsAcousticsAstronomyOpticsComputer science
Has abstract in OpenAlex
yes