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Record W4393221670 · doi:10.3847/2041-8213/ad2df0

First Sagittarius A* Event Horizon Telescope Results. VII. Polarization of the Ring

2024· article· en· W4393221670 on OpenAlexafffund
Kazunori Akiyama, A. Alberdi, W. Alef, Juan Carlos Algaba, Richard Anantua, Keiichi Asada, Rebecca Azulay, U. Bach, Anne-Kathrin Baczko, David Ball, Mislav Baloković, Bidisha Bandyopadhyay, John Barrett, Michi Bauböck, B. A. Benson, Dan Bintley, Lindy Blackburn, R. Blundell, Katherine L. Bouman, Geoffrey C. Bower, Hope Boyce, Michael Bremer, Christiaan D. Brinkerink, Roger Brissenden, S. Britzen, Avery E. Broderick, Dominique Broguière, Thomas Bronzwaer, Sandra Bustamante, Do‐Young Byun, J. E. Carlstrom, Chiara Ceccobello, Andrew Chael, Chi‐kwan Chan, Dominic O. Chang, Koushik Chatterjee, Shami Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, Ilje Cho, Pierre Christian, Nicholas S. Conroy, J. E. Conway, J. M. Cordes, T. M. Crawford, G. Crew, Alejandro Cruz-Osorio, Yuzhu Cui, Rohan Dahale, Jordy Davelaar, Mariafelicia De Laurentis, Roger Deane, Jessica Dempsey, G. Desvignes, Jason Dexter, Vedant Dhruv, Indu K. Dihingia, Sheperd S. Doeleman, Sean Dougal, Sergio A. Dzib, Ralph P. Eatough, Razieh Emami, H. Falcke, Joseph Farah, Vincent L. Fish, E. B. Fomalont, H. Alyson Ford, Marianna Foschi, Raquel Fraga-Encinas, William T. Freeman, Per Friberg, Christian M. Fromm, Antonio Fuentes, Peter Galison, Charles F. Gammie, Roberto García, Olivier Gentaz, Boris Georgiev, C. Goddi, Roman Gold, Arturo I. Gómez-Ruiz, José L. Gómez, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, Daryl Haggard, Kari Haworth, M. H. Hecht, Ronald Hesper, Dirk Heumann, Luis C. Ho, Paul T. P. Ho, Mareki Honma, Lei Huang, D. H. Hughes, Shiro Ikeda, C. M. Violette Impellizzeri, Makoto Inoue, Sara Issaoun, D. J. James, Buell T. Jannuzi, Michaël Janssen, Britton Jeter, Wu Jiang, Alejandra Jiménez-Rosales, Michael D. Johnson, Svetlana G. Jorstad, Abhishek V. Joshi, Taehyun Jung, Mansour Karami, R. Karuppusamy, Tomohisa Kawashima, Garrett K. Keating, Mark Kettenis, Dong-Jin Kim, Jae-Young Kim, Jongsoo Kim, Junhan Kim, Motoki Kino, Jun Yi Koay, Prashant Kocherlakota, Yutaro Kofuji, Patrick M. Koch, Shoko Koyama, C. Krämer, Joana A. Kramer, T. P. Krichbaum, Cheng‐Yu Kuo, Noemi La Bella, Tod R. Lauer, Daeyoung Lee, Sang-Sung Lee, Po Kin Leung, Aviad Levis, Rocco Lico, Greg Lindahl, M. Lindqvist, Mikhail Lisakov, Kuo Liu, Elisabetta Liuzzo, Wen-Ping Lo, A. P. Lobanov, Laurent Loinard, C. J. Lonsdale, A. E. Lowitz, Ru-Sen Lu, Nicholas R. MacDonald, N. Marchili, Sera Markoff, Daniel P. Marrone, Alan P. Marscher, I. Martí‐Vidal, Satoki Matsushita, Lynn D. Matthews, Lia Medeiros, K. M. Menten, Daniel Michalik, Izumi Mizuno, Yosuke Mizuno, J. M. Moran, Kotaro Moriyama, Monika Mościbrodzka, Wanga Mulaudzi, Cornelia Müller, Hendrik Müller, Alejandro Mus, Gibwa Musoke, I. Myserlis, Andrew Nadolski, Hiroshi Nagai, Neil M. Nagar, Masanori Nakamura, Gopal Narayanan, Iniyan Natarajan, Antonios Nathanail, Santiago Navarro Fuentes, Joey Neilsen, R. Neri, Chunchong Ni, A. Noutsos, Michael A. Nowak, Hiroki Okino, Héctor Olivares, Gisela N. Ortiz-León, Tomoaki Oyama, Feryal Özel, Daniel C. M. Palumbo, Georgios Filippos Paraschos, Jongho Park, Harriet Parsons, Nimesh Patel, Ue‐Li Pen, Dominic W. Pesce, Vincent Piétu, R. L. Plambeck, Aleksandar PopStefanija, Oliver Porth, Felix M. Pötzl, Ben Prather, Jorge A. Preciado-López, Dimitrios Psaltis, Hung-Yi Pu, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Alexander W. Raymond, Luciano Rezzolla, Angelo Ricarte, Bart Ripperda, Freek Roelofs, A. E. E. Rogers, Cristina Romero-Cañizales, E. Ros, Arash Roshanineshat, Helge Rottmann, A. L. Roy, Ignacio Ruiz, Chet Ruszczyk, K. L. J. Rygl, Salvador Sánchez, David Sánchez-Argüelles, M. Sánchez‐Portal, Mahito Sasada, Kaushik Satapathy, T. Savolainen, F. Peter Schloerb, Jonathan Schonfeld, K. Schüster, Lijing Shao, Zhi-Qiang Shen, Des Small, Bong Won Sohn, Jason Soohoo, L. Salas, Kamal Souccar, Joshua S. Stanway, He Sun, Fumie Tazaki, Alexandra J. Tetarenko, Paul Tiede, R. P. J. Tilanus, Michael Titus, Pablo Torné, Teresa Toscano, Efthalia Traianou, Tyler Trent, Sascha Trippe, Matthew Turk, Ilse van Bemmel, Huib Jan van Langevelde, Daniel R. van Rossum, Jesse Vos, Jan Wagner, D. Ward–Thompson, J. F. C. Wardle, Jasmin E. Washington, Jonathan Weintroub, Robert Wharton, Maciek Wielgus, K. Wiik, Gunther Witzel, Michael F. Wondrak, George N. Wong, Nitika Yadlapalli, Paul Yamaguchi, Aristomenis Yfantis, Doosoo Yoon, André Young, Ken Young, Ziri Younsi, Wei Yu, J. A. Zensus, Shuo Zhang, Guang-Yao Zhao, Shan-Shan Zhao

Bibliographic record

VenueThe Astrophysical Journal Letters · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of LethbridgeCanadian Institute for Theoretical AstrophysicsUniversity of TorontoPerimeter InstituteUniversity of WaterlooCanadian Institute for Advanced ResearchMcGill University
FundersLos Alamos National LaboratoryOak Ridge National LaboratoryArmy Research OfficeHigh Energy PhysicsNational Key Research and Development Program of ChinaAgencia Estatal de InvestigaciónNational Institutes of Natural SciencesJapan Society for the Promotion of ScienceNational Nuclear Security AdministrationOffice of ScienceToray Science FoundationInstitut Périmètre de physique théoriqueAgencia Nacional de Investigación y DesarrolloIstituto Nazionale di Fisica NucleareShanghai Jiao Tong UniversityCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftGeneralitat ValencianaNational Science FoundationChina Postdoctoral Science FoundationDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekInstituto de Astrofísica de AndalucíaChinese Academy of SciencesFundación Bancaria Caixa d'Estalvis i Pensions de BarcelonaAcademia SinicaJunta de AndalucíaUniversiteit van AmsterdamEuropean Southern ObservatoryNetherlands eScience CenterJohn Templeton FoundationChina Scholarship CouncilMinistry of Education, Culture, Sports, Science and TechnologyRadboud UniversiteitNational Research FoundationCompute CanadaJoint Institute for Computational Fundamental ScienceUniversity of ArizonaSmithsonian InstitutionInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyEuropean CommissionLeverhulme TrustNational Radio Astronomy ObservatoryFundação de Amparo à Pesquisa do Estado de São PauloVetenskapsrådetNational Natural Science Foundation of ChinaU.S. Department of EnergyNational Astronomical Observatory of JapanAssociated UniversitiesConsejo Superior de Investigaciones CientíficasUniversity of ChicagoEast Asian Core Observatories AssociationGordon and Betty Moore FoundationMinisterio de Ciencia, Innovación y UniversidadesNational Aeronautics and Space AdministrationDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoMinisterio de Ciencia e InnovaciónKorea Astronomy and Space Science InstituteScience and Technology Facilities CouncilUniversiteit LeidenFlatiron Health
KeywordsEvent horizonSagittariusPhysicsAstronomyPolarization (electrochemistry)Sagittarius A*TelescopeAstrophysicsHorizonGalactic CenterStarsChemistryMilky Way

Abstract

fetched live from OpenAlex

Abstract The Event Horizon Telescope observed the horizon-scale synchrotron emission region around the Galactic center supermassive black hole, Sagittarius A* (Sgr A*), in 2017. These observations revealed a bright, thick ring morphology with a diameter of 51.8 ± 2.3 μ as and modest azimuthal brightness asymmetry, consistent with the expected appearance of a black hole with mass M ≈ 4 × 10 6 M ⊙ . From these observations, we present the first resolved linear and circular polarimetric images of Sgr A*. The linear polarization images demonstrate that the emission ring is highly polarized, exhibiting a prominent spiral electric vector polarization angle pattern with a peak fractional polarization of ∼40% in the western portion of the ring. The circular polarization images feature a modestly (∼5%–10%) polarized dipole structure along the emission ring, with negative circular polarization in the western region and positive circular polarization in the eastern region, although our methods exhibit stronger disagreement than for linear polarization. We analyze the data using multiple independent imaging and modeling methods, each of which is validated using a standardized suite of synthetic data sets. While the detailed spatial distribution of the linear polarization along the ring remains uncertain owing to the intrinsic variability of the source, the spiraling polarization structure is robust to methodological choices. The degree and orientation of the linear polarization provide stringent constraints for the black hole and its surrounding magnetic fields, which we discuss in an accompanying publication.

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: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.646
Threshold uncertainty score0.456

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 science0.0010.000
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 head0.006
GPT teacher head0.206
Teacher spread0.201 · 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 designBench or experimental
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

Citations103
Published2024
Admission routes2
Has abstractyes

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