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Record W2979599153 · doi:10.1093/mnras/stz2857

The International Pulsar Timing Array: second data release

2019· article· en· W2979599153 on OpenAlexaff
Benetge B. P. Perera, Megan E. DeCesar, Paul B. Demorest, M. Kerr, L. Lentati, David J. Nice, S. Osłowski, S. M. Ransom, M. J. Keith, Zaven Arzoumanian, M. Bailes, P. T. Baker, C. Bassa, N. D. R. Bhat, Adam Brazier, M. Burgay, Sarah Burke-Spolaor, R. N. Caballero, D. J. Champion, Shami Chatterjee, Siyuan Chen, I. Cognard, J. M. Cordes, Kathryn Crowter, Shi Dai, G. Desvignes, Timothy Dolch, R. D. Ferdman, E. C. Ferrara, Emmanuel Fonseca, Janna Goldstein, E. Graikou, L. Guillemot, Jeffrey S. Hazboun, G. Hobbs, H. Hu, Kristina Islo, G. H. Janssen, R. Karuppusamy, M. Krämer, Michael T. Lam, K. J. Lee, Kuan Liu, Jing Luo, A. G. Lyne, R. N. Manchester, James W. McKee, M. A. McLaughlin, Chiara M. F. Mingarelli, A. Parthasarathy, Timothy T. Pennucci, D. Perrodin, Andrea Possenti, Daniel J. Reardon, Craig Russell, S. A. Sanidas, Alberto Sesana, G. Shaifullah, R. M. Shannon, Xavier Siemens, Joseph Simon, R. Spiewak, I. H. Stairs, B. W. Stappers, Joseph K. Swiggum, Stephen R. Taylor, G. Theureau, C. Tiburzi, Michele Vallisneri, A. Vecchio, J B Wang, Songbo Zhang, Lei Zhang, Weiwei Zhu, X. J. Zhu

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoMcGill UniversityUniversity of British ColumbiaCanadian Institute for Advanced Research
FundersAustralian Research CouncilScience and Technology Facilities CouncilSimons FoundationNational Natural Science Foundation of ChinaAustralian GovernmentChinese Academy of SciencesEuropean Research CouncilNational Science Foundation
KeywordsPulsarPhysicsMillisecond pulsarEphemerisObservatoryGravitational waveAstronomyNoise (video)AstrophysicsStatic timing analysisBinary pulsarSatelliteComputer science

Abstract

fetched live from OpenAlex

ABSTRACT In this paper, we describe the International Pulsar Timing Array second data release, which includes recent pulsar timing data obtained by three regional consortia: the European Pulsar Timing Array, the North American Nanohertz Observatory for Gravitational Waves, and the Parkes Pulsar Timing Array. We analyse and where possible combine high-precision timing data for 65 millisecond pulsars which are regularly observed by these groups. A basic noise analysis, including the processes which are both correlated and uncorrelated in time, provides noise models and timing ephemerides for the pulsars. We find that the timing precisions of pulsars are generally improved compared to the previous data release, mainly due to the addition of new data in the combination. The main purpose of this work is to create the most up-to-date IPTA data release. These data are publicly available for searches for low-frequency gravitational waves and other pulsar science.

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)0.003
metaresearch head score (Gemma)0.010
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: none
Teacher disagreement score0.021
Threshold uncertainty score0.072

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.010
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0060.011
Science and technology studies0.0010.000
Scholarly communication0.0030.002
Open science0.0020.003
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0210.039

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 head0.016
GPT teacher head0.281
Teacher spread0.265 · 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

Citations295
Published2019
Admission routes1
Has abstractyes

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Same venueMonthly Notices of the Royal Astronomical SocietySame topicPulsars and Gravitational Waves ResearchFrench-language works237,207