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Record W2181359111 · doi:10.1126/science.aac7087

Resolved magnetic-field structure and variability near the event horizon of Sagittarius A*

2015· article· en· W2181359111 on OpenAlexafffund
Michael D. Johnson, Vincent L. Fish, Sheperd S. Doeleman, Daniel P. Marrone, R. L. Plambeck, J. F. C. Wardle, Kazunori Akiyama, Keiichi Asada, Christopher Beaudoin, Lindy Blackburn, Ray Blundell, Geoffrey C. Bower, Christiaan D. Brinkerink, Avery E. Broderick, R. J. Cappallo, Andrew Chael, G. Crew, Jason Dexter, Matt Dexter, R. Freund, Per Friberg, Roman Gold, Mark Gurwell, Paul T. P. Ho, Mareki Honma, Makoto Inoue, Michael Kosowsky, T. P. Krichbaum, James W. Lamb, Abraham Loeb, Ru-Sen Lu, David H. E. MacMahon, Jonathan C. McKinney, J. M. Moran, Ramesh Narayan, Rurik A. Primiani, Dimitrios Psaltis, A. E. E. Rogers, Katherine Rosenfeld, Jason Soohoo, R. P. J. Tilanus, Michael Titus, Laura Vertatschitsch, Jonathan Weintroub, M. C. H. Wright, Ken Young, J. A. Zensus, L. M. Ziurys

Bibliographic record

VenueScience · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNational Research Council CanadaSmithsonian Astrophysical ObservatoryUniversity of TokyoUniversity of WaterlooNederlandse Organisatie voor Wetenschappelijk OnderzoekIndustry CanadaCalifornia Institute of TechnologyAcademia SinicaNational Aeronautics and Space AdministrationRadboud UniversiteitNatural Sciences and Engineering Research Council of CanadaInstitut Périmètre de physique théoriqueUniversiteit LeidenSmithsonian InstitutionNational Astronomical Observatory of JapanAlexander von Humboldt-StiftungGordon and Betty Moore FoundationGovernment of CanadaNational Science Foundation
KeywordsEvent horizonPhysicsSupermassive black holeAstrophysicsBlack hole (networking)Milky WayAstronomyGalaxySagittarius A*HorizonEvent (particle physics)

Abstract

fetched live from OpenAlex

Near a black hole, differential rotation of a magnetized accretion disk is thought to produce an instability that amplifies weak magnetic fields, driving accretion and outflow. These magnetic fields would naturally give rise to the observed synchrotron emission in galaxy cores and to the formation of relativistic jets, but no observations to date have been able to resolve the expected horizon-scale magnetic-field structure. We report interferometric observations at 1.3-millimeter wavelength that spatially resolve the linearly polarized emission from the Galactic Center supermassive black hole, Sagittarius A*. We have found evidence for partially ordered magnetic fields near the event horizon, on scales of ~6 Schwarzschild radii, and we have detected and localized the intrahour variability associated with these fields.

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
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
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 head0.012
GPT teacher head0.241
Teacher spread0.229 · 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

Citations221
Published2015
Admission routes2
Has abstractyes

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