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Record W4353027542 · doi:10.1093/mnras/stad812

Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

2023· article· en· W4353027542 on OpenAlexafffund
M. Falxa, S. Babak, P. T. Baker, B. Bécsy, A. Chalumeau, Siyuan Chen, Zu-Cheng Chen, Neil J. Cornish, L. Guillemot, Jeffrey S. Hazboun, Chiara M. F. Mingarelli, A. Parthasarathy, Antoine Petiteau, Nihan S. Pol, Alberto Sesana, S. B. Spolaor, Stephen R. Taylor, G. Theureau, Michele Vallisneri, Sarah J. Vigeland, Caitlin A. Witt, X. J. Zhu, John Antoniadis, Zaven Arzoumanian, M. Bailes, N. D. R. Bhat, Laura Blecha, Adam Brazier, Paul R. Brook, R. N. Caballero, A D Cameron, J. Andrew Casey-Clyde, D. J. Champion, Maria Charisi, Shami Chatterjee, I. Cognard, J. M. Cordes, F. Crawford, H. Thankful Cromartie, Kathryn Crowter, Shi Dai, Megan E. DeCesar, Paul B. Demorest, G. Desvignes, Timothy Dolch, Brendan Drachler, Yi Feng, E. C. Ferrara, William Fiore, Emmanuel Fonseca, N. Garver-Daniels, Joseph Glaser, B. Goncharov, Deborah C. Good, J.‐M. Grießmeier, Y. J. Guo, Kayhan Gültekin, G. Hobbs, H. Hu, Kristina Islo, J. Jang, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Jane Kaczmarek, Andrew R. Kaiser, D. L. Kaplan, M. J. Keith, Luke Zoltan Kelley, M. Kerr, J. S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Kuo Liu, Tingting Liu, Jing Luo, Ryan S. Lynch, Dustin R. Madison, Robert Main, R. N. Manchester, Alexander McEwen, James W. McKee, M. A. McLaughlin, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, S. Osłowski, Timothy T. Pennucci, Benetge B. P. Perera, D. Perrodin, N. K. Porayko, Andrea Possenti, H. Quelquejay-Leclere, S. M. Ransom, Paul S. Ray, Daniel J. Reardon, Craig Russell, A. Samajdar, John Sarkissian, Levi Schult, G. Shaifullah, R. M. Shannon, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Tristan L. Smith, Lorenzo Speri, R. Spiewak, I. H. Stairs, B. W. Stappers, Daniel R. Stinebring, Joseph K. Swiggum, C. Tiburzi, Jacob E. Turner, A. Vecchio, J. P. W. Verbiest, Haley M. Wahl, Shuangqiang Wang, J Wang, J. Wang, Ziwei Wu, Lei Zhang, S Zhang

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoHerzberg Institute of AstrophysicsUniversity of British Columbia
FundersU.S. Naval Research LaboratoryOffice of Naval ResearchObservatoire de Paris, Université de Recherche Paris Sciences et LettresScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeHellenic Foundation for Research and InnovationNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueJet Propulsion LaboratoryStavros Niarchos FoundationAgenzia Spaziale ItalianaNuclear Safety and Security CommissionNederlandse Organisatie voor Wetenschappelijk OnderzoekCentre National d’Etudes SpatialesNational Radio Astronomy ObservatoryNational Natural Science Foundation of ChinaH2020 European Research CouncilFlatiron HealthAgence Nationale de la RechercheAustralian GovernmentAssociated UniversitiesAustralian Research CouncilConnecticut Space Grant College ConsortiumSpace Telescope Science InstituteCommonwealth Scientific and Industrial Research OrganisationCanadian Institute for Advanced ResearchASTRONEuropean CommissionCalifornia Institute of TechnologyCollege of Natural Resources and Sciences, Humboldt State UniversityNational Aeronautics and Space AdministrationSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungVanderbilt UniversityGoddard Space Flight CenterMinistero dell’Istruzione, dell’Università e della RicercaBrinson FoundationChina Postdoctoral Science FoundationRegione Autonoma della SardegnaSimons FoundationDeutsche ForschungsgemeinschaftUniversity of Central FloridaRoyal SocietyNational Science Foundation
KeywordsPhysicsPulsarGravitational waveAstrophysicsNoise (video)AstronomyAmplitudeSupermassive black holeOpticsGalaxy

Abstract

fetched live from OpenAlex

ABSTRACT The International Pulsar Timing Array 2nd data release is the combination of data sets from worldwide collaborations. In this study, we search for continuous waves: gravitational wave signals produced by individual supermassive black hole binaries in the local universe. We consider binaries on circular orbits and neglect the evolution of orbital frequency over the observational span. We find no evidence for such signals and set sky averaged 95 per cent upper limits on their amplitude h95. The most sensitive frequency is 10 nHz with h95 = 9.1 × 10−15. We achieved the best upper limit to date at low and high frequencies of the PTA band thanks to improved effective cadence of observations. In our analysis, we have taken into account the recently discovered common red noise process, which has an impact at low frequencies. We also find that the peculiar noise features present in some pulsars data must be taken into account to reduce the false alarm. We show that using custom noise models is essential in searching for continuous gravitational wave signals and setting the upper limit.

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)0.001
metaresearch head score (Gemma)0.004
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 score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.029
GPT teacher head0.315
Teacher spread0.286 · 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

Citations73
Published2023
Admission routes2
Has abstractyes

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