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Record W4387111068 · doi:10.1093/mnras/stad2909

Follow-up analyses to the O3 LIGO–Virgo–KAGRA lensing searches

2023· article· en· W4387111068 on OpenAlexaff
Justin Janquart, M. Wright, Srashti Goyal, C. Chan, A. Ganguly, A. Garron, D. Keitel, A K Y Li, A. Liu, R. K. L. Lo, Anuj Mishra, Anupreeta More, H Phurailatpam, P. Prasia, P. Ajith, S. Biscoveanu, P. Cremonese, J. R. Cudell, José María Ezquiaga, J. García-Bellido, O. A. Hannuksela, K. Haris, I. W. Harry, M. Hendry, S. Husa, Silloo B. Kapadia, T G F Li, I. Magaña Hernandez, Suvodip Mukherjee, E. G. Seo, J. Veitch

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Advanced Research
FundersEuropean Social FundInstitute for Cosmic Ray Research, University of TokyoGreat Southern Development Commission, Government of Western AustraliaAgencia Estatal de InvestigaciónSmithsonian Conservation Biology InstituteNational Science and Technology CouncilEuropean Regional Development FundCentre National de la Recherche ScientifiqueICTP South American Institute for Fundamental ResearchMinistry of Science and ICT, South KoreaNemzeti Kutatási Fejlesztési és Innovációs HivatalNational Research FoundationVlaamse regeringVillum FondenJapan Society for the Promotion of ScienceUniversity Grants CommissionUniversitat de les Illes BalearsNational Astronomical Observatory of JapanDivision of Human Resource DevelopmentKorea Astronomy and Space Science InstituteHungarian Scientific Research FundGeneralitat de CatalunyaGeneralitat ValencianaFonds Wetenschappelijk OnderzoekIstituto Nazionale di Fisica NucleareU.S. Department of EnergyNational Research Foundation of KoreaScottish Universities Physics AllianceNational Natural Science Foundation of ChinaScience and Technology Facilities CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungKorea Institute of Science and Technology InformationNederlandse Organisatie voor Wetenschappelijk OnderzoekDepartment of Atomic Energy, Government of IndiaMinistry of Education, Culture, Sports, Science and TechnologyHorizon 2020 Framework ProgrammeCouncil of Scientific and Industrial Research, IndiaCardiff UniversityAcademia SinicaAbdus Salam International Centre for Theoretical PhysicsLeverhulme TrustEuropean CommissionFonds De La Recherche Scientifique - FNRSRussian Foundation for Basic ResearchCentres de Recerca de CatalunyaInstitut des Origines de LyonRussian Science FoundationScottish Funding CouncilBarcelona Supercomputing CenterMinistry of Education, IndiaUniversidad de MálagaScience and Engineering Research BoardNational Science Foundation
KeywordsPhysicsGravitational microlensingLIGOGravitational lensAstrophysicsDistortion (music)Gravitational waveLens (geology)DetectorAstronomyStrong gravitational lensingOpticsStarsGalaxyRedshiftAmplifier

Abstract

fetched live from OpenAlex

ABSTRACT Along their path from source to observer, gravitational waves may be gravitationally lensed by massive objects leading to distortion in the signals. Searches for these distortions amongst the observed signals from the current detector network have already been carried out, though there have as yet been no confident detections. However, predictions of the observation rate of lensing suggest detection in the future is a realistic possibility. Therefore, preparations need to be made to thoroughly investigate the candidate lensed signals. In this work, we present some follow-up analyses that could be applied to assess the significance of such events and ascertain what information may be extracted about the lens-source system by applying these analyses to a number of O3 candidate events, even if these signals did not yield a high significance for any of the lensing hypotheses. These analyses cover the strong lensing, millilensing, and microlensing regimes. Applying these additional analyses does not lead to any additional evidence for lensing in the candidates that have been examined. However, it does provide important insight into potential avenues to deal with high-significance candidates in future observations.

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)0.002
metaresearch head score (Gemma)0.007
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.007
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0030.003
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0040.001

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 head0.041
GPT teacher head0.335
Teacher spread0.294 · 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 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

Citations52
Published2023
Admission routes1
Has abstractyes

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