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Record W4404720154 · doi:10.1038/s41550-024-02386-6

Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster

2024· article· en· W4404720154 on OpenAlexafffund
Aaron B. Pearlman, Paul Scholz, Suryarao Bethapudi, J. W. T. Hessels, V. M. Kaspi, Franz Kirsten, Kenzie Nimmo, L. G. Spitler, Emmanuel Fonseca, Bradley W. Meyers, I. H. Stairs, Chia Min Tan, Mohit Bhardwaj, Shami Chatterjee, Amanda M. Cook, Alice P. Curtin, Fengqiu Adam Dong, Tarraneh Eftekhari, B. M. Gaensler, Tolga Güver, Jane Kaczmarek, Calvin Leung, Kiyoshi W. Masui, Daniele Michilli, Thomas A. Prince, Ketan R. Sand, Kaitlyn Shin, Kendrick M. Smith, Shriharsh P. Tendulkar

Bibliographic record

VenueNature Astronomy · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Advanced ResearchPerimeter InstituteUniversity of British Columbia, Okanagan CampusCanadian Institute for Theoretical AstrophysicsUniversity of British ColumbiaYork UniversityCentre for Global Health ResearchUniversity of TorontoMcGill University
FundersFonds de recherche du Québec – Nature et technologiesNatural Sciences and Engineering Research Council of CanadaMcGill Space InstituteMax-Planck-GesellschaftUniversity of TorontoSpace Telescope Science InstituteCanada Excellence Research Chairs, Government of CanadaNederlandse Organisatie voor Wetenschappelijk OnderzoekEuropean CommissionMcGill UniversityCanadian Institute for Advanced ResearchCanada Research ChairsNational Aeronautics and Space AdministrationNuclear Safety and Security CommissionUniversiteit van AmsterdamNational Science Foundation
KeywordsMagnetarPhysicsAstrophysicsFast radio burstPulsarGlobular clusterFlareAccretion (finance)AstronomyNeutron starStars

Abstract

fetched live from OpenAlex

The precise origins of fast radio bursts (FRBs) remain unknown. Multiwavelength observations of nearby FRB sources can provide important insights into the enigmatic FRB phenomenon. Here we present results from a sensitive, broadband X-ray and radio observational campaign of FRB 20200120E, the closest known extragalactic repeating FRB source (located 3.63 Mpc away in an ~10-Gyr-old globular cluster). We place deep limits on the persistent and prompt X-ray emission from FRB 20200120E, which we use to constrain possible origins for the source. We compare our results with various classes of X-ray sources, transients and FRB models. We find that FRB 20200120E is unlikely to be associated with ultraluminous X-ray bursts, magnetar-like giant flares or an SGR 1935+2154-like intermediate flare. Although other types of bright magnetar-like intermediate flares and short X-ray bursts would have been detectable from FRB 20200120E during our observations, we cannot entirely rule them out as a class. We show that FRB 20200120E is unlikely to be powered by an ultraluminous X-ray source or a young extragalactic pulsar embedded in a Crab-like nebula. We also provide new constraints on the compatibility of FRB 20200120E with accretion-based FRB models involving X-ray binaries. These results highlight the power of multiwavelength observations of nearby FRBs for discriminating between FRB models.

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: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.789
Threshold uncertainty score0.481

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 science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

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 head0.009
GPT teacher head0.307
Teacher spread0.298 · 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 designNot applicable
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

Citations22
Published2024
Admission routes2
Has abstractyes

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