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Record W2982362750 · doi:10.1093/mnras/stz3071

A pulsar-based time-scale from the International Pulsar Timing Array

2019· article· en· W2982362750 on OpenAlexaff
G. Hobbs, Lei Guo, R. N. Caballero, W. A. Coles, K. J. Lee, R. N. Manchester, Daniel J. Reardon, Demetrios Matsakis, Minglei Tong, Zaven Arzoumanian, M. Bailes, C. Bassa, N. D. R. Bhat, Adam Brazier, Sarah Burke-Spolaor, D. J. Champion, Shami Chatterjee, I. Cognard, Shi Dai, G. Desvignes, Timothy Dolch, R. D. Ferdman, E. Graikou, L. Guillemot, G. H. Janssen, M. J. Keith, M. Kerr, M. Krämer, Michael T. Lam, Kuan Liu, A. G. Lyne, T. Joseph W. Lazio, Ryan S. Lynch, James W. McKee, M. A. McLaughlin, Chiara M. F. Mingarelli, David J. Nice, S. Osłowski, Timothy T. Pennucci, Benetge B. P. Perera, D. Perrodin, Andrea Possenti, Craig Russell, S. A. Sanidas, Alberto Sesana, G. Shaifullah, R. M. Shannon, Joseph Simon, R. Spiewak, I. H. Stairs, B. W. Stappers, Joseph K. Swiggum, Stephen R. Taylor, G. Theureau, Lawrence Toomey, Rutger van Haasteren, Jingbo Wang, Yan Wang, X. J. Zhu

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAdvanced Frequency and Time Standards
Canadian institutionsUniversity of British Columbia
FundersOffice of Experimental Program to Stimulate Competitive ResearchEuropean Research CouncilNational Key Research and Development Program of ChinaScience and Technology Facilities CouncilNational Science Foundation of Sri LankaObservatoire de Paris, Université de Recherche Paris Sciences et LettresJet Propulsion LaboratoryInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftASTRONUniversities Space Research AssociationNational Natural Science Foundation of ChinaFlatiron HealthCommonwealth Scientific and Industrial Research OrganisationAustralian GovernmentCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationNederlandse Organisatie voor Wetenschappelijk OnderzoekNational Science Foundation
KeywordsPulsarPhysicsAstrophysicsObservatoryScale (ratio)Atomic clockGravitational waveStability (learning theory)AstronomyMillisecond pulsarNoise (video)Static timing analysis

Abstract

fetched live from OpenAlex

ABSTRACT We have constructed a new time-scale, TT(IPTA16), based on observations of radio pulsars presented in the first data release from the International Pulsar Timing Array (IPTA). We used two analysis techniques with independent estimates of the noise models for the pulsar observations and different algorithms for obtaining the pulsar time-scale. The two analyses agree within the estimated uncertainties and both agree with TT(BIPM17), a post-corrected time-scale produced by the Bureau International des Poids et Mesures (BIPM). We show that both methods could detect significant errors in TT(BIPM17) if they were present. We estimate the stability of the atomic clocks from which TT(BIPM17) is derived using observations of four rubidium fountain clocks at the US Naval Observatory. Comparing the power spectrum of TT(IPTA16) with that of these fountain clocks suggests that pulsar-based time-scales are unlikely to contribute to the stability of the best time-scales over the next decade, but they will remain a valuable independent check on atomic time-scales. We also find that the stability of the pulsar-based time-scale is likely to be limited by our knowledge of solar-system dynamics, and that errors in TT(BIPM17) will not be a limiting factor for the primary goal of the IPTA, which is to search for the signatures of nano-Hertz gravitational waves.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.005
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0020.003
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0050.001

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 head0.006
GPT teacher head0.212
Teacher spread0.206 · 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

Citations96
Published2019
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicAdvanced Frequency and Time StandardsFrench-language works237,207