MétaCan
Menu
Back to cohort
Record W4224116161 · doi:10.1051/0004-6361/202143006

TRAPUM discovery of 13 new pulsars in NGC 1851 using MeerKAT

2022· article· en· W4224116161 on OpenAlexfundno aff
A. Ridolfi, P. C. C. Freire, T. Gautam, S. M. Ransom, E D Barr, S. Buchner, M. Burgay, Federico Abbate, V. Venkatraman Krishnan, L Vleeschower, Andrea Possenti, B. W. Stappers, W Chen, P V Padmanabh, D. J. Champion, M. Bailes, L. Levin, E. F. Keane, R. P. Breton, M C Bezuidenhout, J.‐M. Grießmeier, Lars Künkel, Yunpeng Men, F. Camilo, M. Geyer, B. Hugo, A. Jameson, A. Parthasarathy, M. Serylak

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersMinistero degli Affari Esteri e della Cooperazione InternazionaleMax-Planck-GesellschaftFP7 International CooperationScience and Technology Facilities CouncilNational Research FoundationEuropean CommissionObservatoire de Paris, Université de Recherche Paris Sciences et LettresUniversity of ManchesterAustralian GovernmentAssociated UniversitiesTata Institute of Fundamental ResearchCanadian Institute for Advanced ResearchSwinburne University of TechnologyNational Radio Astronomy ObservatoryNational Science Foundation
KeywordsGlobular clusterPulsarPhysicsMillisecond pulsarAstrophysicsNeutron starAstronomyCluster (spacecraft)PopulationStarsComputer science

Abstract

fetched live from OpenAlex

We report the discovery of 13 new pulsars in the globular cluster NGC 1851 by the TRAPUM Large Survey Project using the MeerKAT radio telescope. The discoveries consist of six isolated millisecond pulsars (MSPs) and seven binary pulsars, of which six are MSPs and one is mildly recycled. For all the pulsars, we present the basic kinematic, astrometric, and orbital parameters, where applicable, as well as their polarimetric properties, when these are measurable. Two of the binary MSPs (PSR J0514−4002D and PSR J0514−4002E) are in wide and extremely eccentric (e > 0.7) orbits with a heavy white dwarf and a neutron star as their companion, respectively. With these discoveries, NGC 1851 is now tied with M28 as the cluster with the third largest number of known pulsars (14). Its pulsar population shows remarkable similarities with that of M28, Terzan 5, and other clusters with comparable structural parameters. The newly found pulsars are all located in the innermost regions of NGC 1851 and will likely enable, among other things, detailed studies of the cluster structure and dynamics.

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)0.000
metaresearch head score (Gemma)0.000
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 score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
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 head0.014
GPT teacher head0.287
Teacher spread0.273 · 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

Citations38
Published2022
Admission routes1
Has abstractyes

Explore more

Same venueAstronomy and AstrophysicsSame topicPulsars and Gravitational Waves ResearchFrench-language works237,207