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Record W4282930996 · doi:10.1038/s41586-022-04755-5

A repeating fast radio burst associated with a persistent radio source

2022· article· en· W4282930996 on OpenAlexafffund
C.-H. Niu, K.K. Aggarwal, Di Li, Xian Zhang, Shami Chatterjee, Chris Tsai, Wenfei Yu, Casey Law, Sarah Burke-Spolaor, J. M. Cordes, Yongkun Zhang, Stella Koch Ocker, Jumei Yao, P. Wang, Yi Feng, Yuu Niino, Christopher D. Bochenek, Marilyn Cruces, Liam Connor, J.-A. Jiang, Shi Dai, Rui Luo, Guodong Li, Caixia Miao, Jiarui Niu, Reshma Anna-Thomas, Jessica Sydnor, Daniel Stern, Weiyang Wang, Mao Yuan, Youling Yue, D. J. Zhou, Zhen Yan, Weiwei Zhu, Bing Zhang

Bibliographic record

VenueNature · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Advanced Research
FundersNational Astronomical Observatory of JapanNational Natural Science Foundation of ChinaNational Radio Astronomy ObservatoryCanadian Institute for Advanced ResearchJapan Society for the Promotion of ScienceNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyAustralian GovernmentAssociated UniversitiesW. M. Keck FoundationNational Science Foundation
KeywordsAstrophysicsPhysicsFast radio burstIntergalactic travelRedshiftGalaxyDispersion (optics)Radio galaxyQuasarX-shaped radio galaxyAstronomyOptics

Abstract

fetched live from OpenAlex

Abstract The dispersive sweep of fast radio bursts (FRBs) has been used to probe the ionized baryon content of the intergalactic medium 1 , which is assumed to dominate the total extragalactic dispersion. Although the host-galaxy contributions to the dispersion measure appear to be small for most FRBs 2 , in at least one case there is evidence for an extreme magneto-ionic local environment 3,4 and a compact persistent radio source 5 . Here we report the detection and localization of the repeating FRB 20190520B, which is co-located with a compact, persistent radio source and associated with a dwarf host galaxy of high specific-star-formation rate at a redshift of 0.241 ± 0.001. The estimated host-galaxy dispersion measure of approximately $${903}_{-111}^{+72}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mrow> <mml:mn>903</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>111</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>72</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> parsecs per cubic centimetre, which is nearly an order of magnitude higher than the average of FRB host galaxies 2,6 , far exceeds the dispersion-measure contribution of the intergalactic medium. Caution is thus warranted in inferring redshifts for FRBs without accurate host-galaxy identifications.

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 score0.371
Threshold uncertainty score0.811

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 integrity0.0000.002
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 head0.007
GPT teacher head0.271
Teacher spread0.264 · 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

Citations284
Published2022
Admission routes2
Has abstractyes

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