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Record W4280648529 · doi:10.3847/2041-8213/ac6736

First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass

2022· article· en· W4280648529 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
fundA Canadian funder is recorded on the work.

Bibliographic record

VenueThe Astrophysical Journal Letters · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoPerimeter InstituteUniversity of WaterlooCanadian Institute for Advanced ResearchMcGill University
FundersLos Alamos National LaboratoryOak Ridge National LaboratoryAstrophysics DivisionOffice of International Science and EngineeringNational Key Research and Development Program of ChinaJapan Society for the Promotion of SciencePhysics Division, National Center for Theoretical SciencesNational Nuclear Security AdministrationToray Science FoundationEast Asian Core Observatories AssociationInstitut Périmètre de physique théoriqueAgencia Nacional de Investigación y DesarrolloIstituto Nazionale di Fisica NucleareNational Astronomical Observatory of JapanUniversidad Nacional Autónoma de MéxicoRecruitment Program of Global ExpertsShanghai Jiao Tong UniversityAcademy of FinlandMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueMinistry of Education, IndiaNational Natural Science Foundation of ChinaNational Research Foundation of KoreaMinisterio de Ciencia, Innovación y UniversidadesNuclear Safety and Security CommissionGeneralitat ValencianaNational Science FoundationChina Postdoctoral Science FoundationInstituto de Astrofísica de AndalucíaDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekChinese Academy of SciencesAcademia SinicaJunta de AndalucíaUniversiteit van AmsterdamNatural Sciences and Engineering Research Council of CanadaNetherlands eScience CenterEuropean Southern ObservatoryJohn Templeton FoundationChina Scholarship CouncilMinistry of Education, Culture, Sports, Science and TechnologyRadboud UniversiteitUniversity of PretoriaNational Research FoundationCompute CanadaOffice of ScienceSimons FoundationJoint Institute for Computational Fundamental ScienceUniversity of ArizonaSmithsonian InstitutionInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyVetenskapsrådetU.S. Department of EnergyEuropean CommissionLeverhulme TrustNational Radio Astronomy ObservatoryKorea Astronomy and Space Science InstituteScience and Technology Facilities CouncilUniversiteit LeidenAssociated UniversitiesSpace Telescope Science InstituteUniversitat de ValènciaNational Center for Theoretical SciencesNational Institutes of Natural SciencesGovernment of CanadaDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoMinisterio de Ciencia e InnovaciónConsejo Nacional de Ciencia y TecnologíaConsejo Superior de Investigaciones CientíficasUniversity of ChicagoNational Aeronautics and Space AdministrationGordon and Betty Moore FoundationFlatiron Health
KeywordsPhysicsSagittarius A*AstrophysicsRADIUSCalibrationSupermassive black holeGalaxy

Abstract

fetched live from OpenAlex

Abstract In this paper we quantify the temporal variability and image morphology of the horizon-scale emission from Sgr A*, as observed by the EHT in 2017 April at a wavelength of 1.3 mm. We find that the Sgr A* data exhibit variability that exceeds what can be explained by the uncertainties in the data or by the effects of interstellar scattering. The magnitude of this variability can be a substantial fraction of the correlated flux density, reaching ∼100% on some baselines. Through an exploration of simple geometric source models, we demonstrate that ring-like morphologies provide better fits to the Sgr A* data than do other morphologies with comparable complexity. We develop two strategies for fitting static geometric ring models to the time-variable Sgr A* data; one strategy fits models to short segments of data over which the source is static and averages these independent fits, while the other fits models to the full data set using a parametric model for the structural variability power spectrum around the average source structure. Both geometric modeling and image-domain feature extraction techniques determine the ring diameter to be 51.8 ± 2.3 μ as (68% credible intervals), with the ring thickness constrained to have an FWHM between ∼30% and 50% of the ring diameter. To bring the diameter measurements to a common physical scale, we calibrate them using synthetic data generated from GRMHD simulations. This calibration constrains the angular size of the gravitational radius to be <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mrow> <mml:mn>4.8</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.7</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>1.4</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> μ as, which we combine with an independent distance measurement from maser parallaxes to determine the mass of Sgr A* to be <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mrow> <mml:mn>4.0</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.6</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>1.1</mml:mn> </mml:mrow> </mml:msubsup> <mml:mo>×</mml:mo> <mml:msup> <mml:mrow> <mml:mn>10</mml:mn> </mml:mrow> <mml:mrow> <mml:mn>6</mml:mn> </mml:mrow> </mml:msup> </mml:math> M ⊙ .

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.

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 categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.503
Threshold uncertainty score1.000

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 studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.000
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 head0.010
GPT teacher head0.219
Teacher spread0.209 · 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