MétaCan
Menu
Back to cohort
Record W4398229869 · doi:10.3847/2041-8213/ad6572

Swift J1727.8–1613 Has the Largest Resolved Continuous Jet Ever Seen in an X-Ray Binary

2024· preprint· en· W4398229869 on OpenAlexafffund
Callan M. Wood, J. C. A. Miller‐Jones, Arash Bahramian, S. J. Tingay, Steve Prabu, T. D. Russell, P. Atri, Francesco Carotenuto, D. Altamirano, S. Motta, Lucas J. Hyland, Cormac Reynolds, Stuart Weston, R. P. Fender, Elmar Körding, D. Maitra, Sera Markoff, S. Migliari, D. M. Russell, Craig L. Sarazin, G. R. Sivakoff, Roberto Soria, Alexandra J. Tetarenko, V. Tudose

Bibliographic record

VenueThe Astrophysical Journal Letters · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsUniversity of LethbridgeUniversity of Alberta
FundersRIKENSwinburne University of TechnologyTamkeenJapan Aerospace Exploration AgencyNew York University Abu DhabiCommonwealth Scientific and Industrial Research OrganisationAustralian GovernmentScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaAuckland University of Technology, New ZealandGovernment of Western AustraliaNational Science Foundation
KeywordsSwiftJet (fluid)Binary numberX-rayPhysicsMaterials scienceAstrophysicsMathematicsNuclear physicsMechanicsArithmetic

Abstract

fetched live from OpenAlex

Abstract Multiwavelength polarimetry and radio observations of Swift J1727.8–1613 at the beginning of its recent 2023 outburst suggested the presence of a bright compact jet aligned in the north–south direction, which could not be confirmed without high-angular-resolution images. Using the Very Long Baseline Array and the Long Baseline Array, we imaged Swift J1727.8–1613 during the hard/hard-intermediate state, revealing a bright core and a large, two-sided, asymmetrical, resolved jet. The jet extends in the north–south direction, at a position angle of −0.60° ± 0.07° east of north. At 8.4 GHz, the entire resolved jet structure is <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mo>∼</mml:mo> <mml:mn>110</mml:mn> <mml:mo stretchy="false">(</mml:mo> <mml:mi>d</mml:mi> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:mn>2.7</mml:mn> <mml:mspace width="0.25em"/> <mml:mi>kpc</mml:mi> <mml:mo stretchy="false">)</mml:mo> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:mi>sin</mml:mi> <mml:mi>i</mml:mi> </mml:math> au long, with the southern approaching jet extending <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mo>∼</mml:mo> <mml:mn>80</mml:mn> <mml:mo stretchy="false">(</mml:mo> <mml:mi>d</mml:mi> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:mn>2.7</mml:mn> <mml:mspace width="0.25em"/> <mml:mi>kpc</mml:mi> <mml:mo stretchy="false">)</mml:mo> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:mi>sin</mml:mi> <mml:mi>i</mml:mi> </mml:math> au from the core, where d is the distance to the source and i is the inclination of the jet axis to the line of sight. These images reveal the most resolved continuous X-ray binary jet, and possibly the most physically extended continuous X-ray binary jet ever observed. Based on the brightness ratio of the approaching and receding jets, we put a lower limit on the intrinsic jet speed of β ≥ 0.27 and an upper limit on the jet inclination of i ≤ 74°. In our first observation we also detected a rapidly fading discrete jet knot 66.89 ± 0.04 mas south of the core, with a proper motion of 0.66 ± 0.05 mas hr −1 , which we interpret as the result of a downstream internal shock or a jet–interstellar medium interaction, as opposed to a transient relativistic jet launched at the beginning of the outburst.

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 categoriesMeta-epidemiology (narrow), Scholarly communication, Research integrity
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.689
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.000
Science and technology studies0.0010.001
Scholarly communication0.0010.000
Open science0.0020.001
Research integrity0.0000.006
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 head0.021
GPT teacher head0.246
Teacher spread0.226 · 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.

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

Citations34
Published2024
Admission routes2
Has abstractyes

Explore more

Same venueThe Astrophysical Journal LettersSame topicAstrophysical Phenomena and ObservationsFrench-language works237,207