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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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.114
Threshold uncertainty score0.781

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0020.001
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 head0.016
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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
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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