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Record W2785157674 · doi:10.1103/physrevd.97.082002

Identification and mitigation of narrow spectral artifacts that degrade searches for persistent gravitational waves in the first two observing runs of Advanced LIGO

2018· article· en· W2785157674 on OpenAlexafffund
P. B. Covas, A. Effler, E. Goetz, P. M. Meyers, A. Neunzert, M. Oliver, B. L. Pearlstone, V. J. Roma, R. M. S. Schofield, V. B. Adya, P. Astone, S. Biscoveanu, T. A. Callister, N. Christensen, A. Colla, E. Coughlin, M. W. Coughlin, S. G. Crowder, S. E. Dwyer, H.‐B. Eggenstein, S. Hourihane, S. Kandhasamy, Wei Liu, A. P. Lundgren, A. Matas, R. McCarthy, J. McIver, G. Mendell, R. G. Ormiston, C. Palomba, M. A. Papa, O. J. Piccinni, K. Rao, K. Riles, L. Sammut, S. Schlassa, D. Sigg, N. A. Strauss, D. Tao, K. A. Thorne, E. Thrane, S. Trembath-reichert, B. P. Abbott, R. Abbott, T. D. Abbott, C. Adams, A. Ananyeva, S. Appert, K. Arai, Stuart Aston, C. Austin, S. Ballmer, D. Barker, B. Barr, L. Barsotti, J. Bartlett, I. Bartos, J. C. Batch, M. Bejger, A. S. Bell, J. Betzwieser, G. Billingsley, J. Birch, Sébastien Biscans, C. Biwer, C. D. Blair, R. M. Blair, R. Bork, A. F. Brooks, H. Cao, G. Ciani, F. Clara, P. Clearwater, S. J. Cooper, P. Corban, S. T. Countryman, M. J. Cowart, D. C. Coyne, A. Cumming, L. Cunningham, K. Danzmann, C. F. Da Silva Costa, E. J. Daw, D. DeBra, R. T. DeRosa, R. DeSalvo, K. L. Dooley, S. Doravari, J. C. Driggers, T. B. Edo, T. Etzel, M. Evans, T. Evans, M. Factourovich, H. Fair, A. Fernández Galiana, E. C. Ferreira, R. P. Fisher, R. Frey, P. Fritschel, V. V. Frolov, P. Fulda, M. Fyffe, B. Gateley, J. A. Giaime, K. D. Giardina, B. Goncharov, S. Gras, C. Gray, H. Grote, K. E. Gushwa, E. K. Gustafson, R. Gustafson, E. D. Hall, G. Hammond, J. Hanks, J. Hanson, T. Hardwick, I. W. Harry, M. C. Heintze, A. Heptonstall, J. Hough, R. Inta, K. Izumi, R. Jones, S. Karki, M. Kasprzack, S. Kaufer, K. Kawabe, R. Kennedy, N. Kijbunchoo, W. Kim, E. J. King, P. J. King, J. S. Kissel, W. Z. Korth, G. Kuehn, M. Landry, B. Lantz, M. Laxen, J. Liu, N. A. Lockerbie, M. Lormand, M. MacInnis, D. M. Macleod, Szabolcs Márka, Z. Márka, A. S. Markosyan, E. Maros, P. Marsh, I. W. Martin, Д. В. Мартынов, K. Mason, T. J. Massinger, F. Matichard, N. Mavalvala, D. E. McClelland, S. McCormick, L. McCuller, G. McIntyre, T. McRae, E. L. Merilh, J. Miller, R. Mittleman, Geoffrey Mo, K. Mogushi, D. Moraru, G. Moreno, Guido Mueller, N. Mukund, A. Mullavey, J. Munch, T. J. N. Nelson, P. Nguyen, L. K. Nuttall, J. Oberling, O. Oktavia, P. Oppermann, Richard J. Oram, B. O’Reilly, D. J. Ottaway, H. Overmier, J. R. Palamos, W. Parker, A. Pele, S. Penn, C. J. Perez, M. Phelps, V. Pierro, I. M. Pinto, M. Principe, L. Prokhorov, O. Puncken, V. Quetschke, E. A. Quintero, H. Radkins, P. Raffai, K. E. Ramirez, S. Reid, D. H. Reitze, N. A. Robertson, J. G. Rollins, C. L. Romel, J. H. Romie, M. P. Ross, S. Rowan, K. Ryan, T. Sadecki, E. J. Sanchez, L. E. Sanchez, V. Sandberg, R. L. Savage, D. Sellers, D. A. Shaddock, Thomas Shaffer, B. Shapiro, D. H. Shoemaker, B. J. J. Slagmolen, J. R. Smith, B. Sorazu, A. P. Spencer, A. Staley, K. A. Strain, L. Sun, D. B. Tanner, Jay D. Tasson, Richard W. Taylor, Michael Thomas, P. Thomas, K. Toland, C. I. Torrie, G. Traylor, M. Tse, D. Tuyenbayev, G. Vajente, G. Valdes, A. A. van Veggel, A. Vecchio, P. J. Veitch, K. Venkateswara, T. Vo, C. Vorvick, M. Wade, M. Walker, R. L. Ward, J. Warner, B. Weaver, R. Weiss, P. Weßels, B. Willke, C. C. Wipf, J. K. Wofford, J. Worden, H. Yamamoto, C. C. Yancey, Hang Yu, Haocun Yu, L. Zhang, S. J. Zhu, M. E. Zucker, J. Zweizig

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersAustralian Research CouncilScience and Technology Facilities CouncilMinistry of Science and Technology, TaiwanMinistry of Education, IndiaConseil Régional, Île-de-FranceNational Research Foundation of KoreaConselleria d'Educació, Investigació, Cultura i EsportMinistério da Ciência, Tecnologia e InovaçãoHungarian Scientific Research FundGeneralitat ValencianaIndustry CanadaKavli FoundationNational Natural Science Foundation of ChinaNational Research, Development and Innovation OfficeAgencia Estatal de InvestigaciónSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungGovern de les Illes BalearsNederlandse Organisatie voor Wetenschappelijk OnderzoekRussian Foundation for Basic ResearchResearch Grants Council, University Grants CommitteeCentre National de la Recherche ScientifiqueCouncil of Scientific and Industrial Research, IndiaNational Research FoundationNemzeti Kutatási Fejlesztési és Innovációs HivatalAbdus Salam International Centre for Theoretical PhysicsInstituto Nazionale di Fisica NucleareEuropean CommissionDivision of Human Resource DevelopmentCanadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of CanadaICTP South American Institute for Fundamental ResearchCanadian Institute for Advanced ResearchMinistero dello Sviluppo EconomicoInstitut des Origines de LyonRussian Science FoundationLeverhulme TrustScottish Funding CouncilEuropean Regional Development FundScottish Universities Physics AllianceIstituto Nazionale di Fisica NucleareDepartment of Science and Technology, Ministry of Science and Technology, IndiaOntario Ministry of Economic Development and InnovationScience and Engineering Research BoardNational Science FoundationMax-Planck-GesellschaftRoyal SocietyResearch Corporation for Science Advancement
KeywordsLIGOGravitational waveNeutron starPhysicsSuperposition principleIdentification (biology)AstrophysicsAstronomyAsteroseismologyGravitational-wave astronomyStars

Abstract

fetched live from OpenAlex

Searches are under way in Advanced LIGO and Virgo data for persistent gravitational waves from continuous sources, e.g. rapidly rotating galactic neutron stars, and stochastic sources, e.g. relic gravitational waves from the Big Bang or superposition of distant astrophysical events such as mergers of black holes or neutron stars. These searches can be degraded by the presence of narrow spectral artifacts (lines) due to instrumental or environmental disturbances. We describe a variety of methods used for finding, identifying and mitigating these artifacts, illustrated with particular examples. Results are provided in the form of lists of line artifacts that can safely be treated as non-astrophysical. Such lists are used to improve the efficiencies and sensitivities of continuous and stochastic gravitational wave searches by allowing vetoes of false outliers and permitting data cleaning.

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)0.008
metaresearch head score (Gemma)0.025
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.040

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0080.025
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.004
Science and technology studies0.0010.001
Scholarly communication0.0030.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.001

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 head0.039
GPT teacher head0.454
Teacher spread0.415 · 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".

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Citations148
Published2018
Admission routes2
Has abstractyes

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Same venuePhysical review. D/Physical review. D.Same topicPulsars and Gravitational Waves ResearchFrench-language works237,207