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Record W4413084389 · doi:10.3847/1538-4357/ade2e6

Comprehensive Radio Monitoring of the Black Hole X-Ray Binary Swift J1727.8−1613 during Its 2023–2024 Outburst

2025· article· en· W4413084389 on OpenAlexfundno aff
A.K. Hughes, Francesco Carotenuto, Alexandra J. Tetarenko, J. C. A. Miller‐Jones, Arash Bahramian, Joe Bright, F. J. Cowie, Rob Fender, Mark Gurwell, Jasvinderjit K. Khaulsay, Elodie Lescure, Michael L. McCollough, Richard M. Plotkin, Ramprasad Rao, S. D. Vrtilek, D. R. Williams, Callan M. Wood, G. R. Sivakoff, D. Altamirano, P. Casella, S. Corbel, David R. DeBoer, M. Del Santo, Constanza Echiburú-Trujillo, Wael Farah, P. Gandhi, K. I. I. Koljonen, Thomas J. Maccarone, James Matthews, Sera Markoff, Alexander W. Pollak, D. M. Russell, Payaswini Saikia, Noel Castro Segura, A. W. Shaw, Andrew Siemion, Roberto Soria, John A. Tomsick, J. van den Eijnden

Bibliographic record

VenueThe Astrophysical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersSmithsonian Astrophysical ObservatoryUniversity of Cape TownEuropean CommissionINAF - Osservatorio Astrofisico di CataniaNational Astronomical Observatory of JapanRIKENKorea Astronomy and Space Science InstituteNational Institutes of Natural SciencesHORIZON EUROPE Framework ProgrammeUniversity of the Western CapeCanada Research ChairsAustralian GovernmentJapan Aerospace Exploration AgencyCommonwealth Scientific and Industrial Research OrganisationAcademia SinicaNational Science FoundationUK Research and InnovationNational Research FoundationUniversity of PretoriaUniversity of WarwickSmithsonian InstitutionNational Radio Astronomy ObservatoryScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of Canada
KeywordsPhysicsAstrophysicsLight curveSwiftAstronomyBlack hole (networking)Radiative transfer

Abstract

fetched live from OpenAlex

Abstract This work presents comprehensive multifrequency radio monitoring of the black hole low-mass X-ray binary (LMXB) Swift J1727.8−1613, which underwent its first recorded outburst after its discovery in 2023 August. Through a considerable community effort, we have coalesced the data from multiple, distinct observing programs; the light curves include ∼10 months and 197 epochs of monitoring from seven radio facilities with observing frequencies ranging from (approximately) 0.3–230 GHz. The primary purpose of this work is to provide the broader astronomical community with these light curves to assist with the interpretation of other observing campaigns, particularly nonradio observing frequencies. We discuss the phenomenological evolution of the source, which included (i) multiple radio flares consistent with the launching of discrete jet ejections, the brightest of which reached ∼1 Jy; (ii) temporally evolving radio spectral indices ( α ), reaching values steeper than expected for optically thin synchrotron emission ( α < −1) and emission with significant radiative cooling ( α < −1.5). We have published a digital copy of the data and intend for this work to set a precedent for the community to continue releasing comprehensive radio light curves of future LMXB outbursts.

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 score0.009
Threshold uncertainty score0.018

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 communication0.0000.000
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 head0.015
GPT teacher head0.247
Teacher spread0.232 · 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

Citations3
Published2025
Admission routes1
Has abstractyes

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