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Record W4416821274 · doi:10.1051/0004-6361/202556759

Full-polarization millimeter wavelength variability of Sagittarius A <sup>*</sup> during the 2018 EHT campaign

2025· article· en· W4416821274 on OpenAlexafffund
Ezequiel Albentosa-Ruíz, E. Washington, N. Marchili, Iván Martí-Vidal, C. Goddi, Maciek Wielgus, Alejandro Mus, Angelo Ricarte, Daniel P. Marrone, D.S. León Salas, Yuhei Iwata, Alexandra J. Tetarenko, Kotaro Moriyama, Vedant Dhruv, Kazunori Akiyama, A. Alberdi, Walter 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, Amy Benson, Dan Bintley, Lindy Blackburn, R. Blundell, L. Katherine Bouman, Geoffrey C. Bower, Michael Bremer, Roger Brissenden, S. Britzen, E. Avery Broderick, Dominique Broguière, Thomas Bronzwaer, Sandra Bustamante, Andrew Chael, Chi‐kwan Chan, O. Chang, Koushik Chatterjee, Shami Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, Pierre Christian, Ilje Cho, S. Nicholas Conroy, J. E. Conway, M. K. Crawford, G. Crew, Alejandro Cruz-Osorio, Yuzhu Cui, Brandon Curd, Rohan Dahale, Jordy Davelaar, Mariafelicia De Laurentis, Roger Deane, Jessica Dempsey, G. Desvignes, Jason Dexter, Indu K. Dihingia, Sheperd S. Doeleman, A. Sergio Dzib, Ralph P. Eatough, Razieh Emami, H. Falcke, Joseph Farah, E. B. Fomalont, H. Alyson Ford, Marianna Foschi, Antonio Fuentes, Raquel Fraga-Encinas, Per Friberg, Peter Galison, Charles F. Gammie, Roberto García, Olivier Gentaz, Gertie Geertsema, Boris Georgiev, Roman Gold, I. Arturo Gómez-Ruiz, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, Daryl Haggard, Ronald Hesper, Dirk Heumann, Paul T. P. Ho, Mareki Honma, Lei Huang, Shiro Ikeda, C. M. Violette Impellizzeri, Makoto Inoue, Sara Issaoun, J. David James, Buell T. Jannuzi, Michaël Janssen, Britton Jeter, Wu Jiang, Alejandra Jiménez-Rosales, D.M. Johnson, C. Adam Jones, Taehyun Jung, R. Karuppusamy, Tomohisa Kawashima, Katie M. Keating, Mark Kettenis, Dong-Jin Kim, Jae-Young Kim, Jongsoo Kim, Junhan Kim, Motoki Kino, Jun Yi Koay, Prashant Kocherlakota, Yutaro Kofuji, Shoko Koyama, C. Krämer, M. Kramer, P. Thomas Krichbaum, Cheng‐Yu Kuo, Noemi La Bella, Sang-Sung Lee, Aviad Levis, Zhi‐Yuan Li, Rocco Lico, Greg Lindahl, M. Lindqvist, Mikhail Lisakov, Kuo Liu, Elisabetta Liuzzo, Wen-Ping Lo, A. P. Lobanov, Laurent Loinard, A. E. Lowitz, Ru-Sen Lu, R. Nicholas MacDonald, Jirong Mao, Sera Markoff, Alan P. Marscher, Satoki Matsushita, Lia Medeiros, M. Karl Menten, Izumi Mizuno, Yosuke Mizuno, J. Montgomery, Monika Mościbrodzka, Wanga Mulaudzi, Hendrik Müller, Cornelia Müller, I. Myserlis, Hiroshi Nagai, Greshma Nair, Masanori Nakamura, Gopal Narayanan, Iniyan Natarajan, Antonios Nathanail, Santiago Navarro Fuentes, Joey Neilsen, Chunchong Ni, Hiroki Okino, Héctor Olivares, Tomoaki Oyama, Feryal Özel, Georgios Filippos Paraschos, Jongho Park, Harriet Parsons, Nimesh Patel, Ue‐Li Pen, Dominic W. Pesce, Vincent Piétu, Aleksandar PopStefanija, Oliver Porth, Ben Prather, G. Principe, Hung-Yi Pu, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Luciano Rezzolla, Bart Ripperda, Jan Röder, Freek Roelofs, Cristina Romero-Cañizales, E. Ros, Arash Roshanineshat, Helge Rottmann, Ignacio Ruiz, Chet Ruszczyk, L.J. Kazi Rygl, Salvador Sánchez, David Sánchez-Argüelles, Miguel Sánchez-Portal, Mahito Sasada, Kaushik Satapathy, Saurabh Kumar, T. Savolainen, F. Peter Schloerb, Jonathan Schonfeld, K. Schüster, Lijing Shao, Zhiqiang Shen, S. Silpa, Des Small, Bong Won Sohn, Jason Soohoo, Kamal Souccar, Joshua S. Stanway, He Sun, Fumie Tazaki, Paul Tiede, R. P. J. Tilanus, Michael S. Titus, Kenji Toma, 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, Robert Wharton, K. Wiik, Gunther Witzel, F. Michael Wondrak, N. George Wong, Qingwen Wu, Nitika Yadlapalli, Paul Yamaguchi, Aristomenis Yfantis, Doosoo Yoon, André Young, Ziri Younsi, Wei Yu, Ai-Ling Zeng, J. A. Zensus, Shuo Zhang, Guang-Yao Zhao, Shan-Shan Zhao

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoCanadian Institute for Advanced ResearchTrinity CollegeMcGill UniversityPerimeter InstituteUniversity of WaterlooUniversity of Lethbridge
FundersLos Alamos National LaboratoryHigh Energy PhysicsOffice of International Science and EngineeringAgencia Estatal de InvestigaciónEuropean Social FundConsejo Superior de Investigaciones CientíficasFundação para a Ciência e a TecnologiaVetenskapsrådetFonds de recherche du Québec – Nature et technologiesScience and Technology Facilities CouncilHORIZON EUROPE Framework ProgrammeInstitut Périmètre de physique théoriqueNational Science and Technology CouncilAgencia Nacional de Investigación y DesarrolloMinistry of Science and ICT, South KoreaJunta de AndalucíaNational Astronomical Observatory of JapanDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoMinisterio de Ciencia e InnovaciónChina Scholarship CouncilJohn Templeton FoundationMinistry of Education, Culture, Sports, Science and TechnologyNatural Sciences and Engineering Research Council of CanadaMinistry of Education, IndiaMax-Planck-GesellschaftKorea Astronomy and Space Science InstituteGeneralitat ValencianaDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekJapan Society for the Promotion of ScienceCanada Research ChairsSmithsonian InstitutionInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyNational Science FoundationChina Postdoctoral Science FoundationCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorLeverhulme TrustNational Radio Astronomy ObservatoryFundação de Amparo à Pesquisa do Estado de São PauloU.S. Department of EnergyToray Science FoundationUniversity of PretoriaJoint Institute for Computational Fundamental ScienceNational Center for Theoretical SciencesEast Asian Core Observatories AssociationNational Institutes of Natural SciencesGovernment of CanadaGordon and Betty Moore FoundationCERNNational Aeronautics and Space AdministrationAcademia SinicaSmithsonian Astrophysical ObservatoryFlatiron Health
KeywordsSupermassive black holeMillimeterFlareLight curvePolarization (electrochemistry)Accretion (finance)Milky WayEvent horizonTelescopePolarization in astronomy

Abstract

fetched live from OpenAlex

Context. Sagittarius A* (Sgr A * ), the supermassive black hole at the center of the Milky Way, provides a unique laboratory to study accretion dynamics and plasma processes near the event horizon. Aims. We investigated the variability and polarization properties of Sgr A * using ALMA observations during the 2018 Event Horizon Telescope campaign. Methods. We analyzed high-cadence full-polarization light curves from ALMA at millimeter wavelengths, performed time-series analysis, and investigated the temporal behavior during an X-ray flare observed by Chandra on 2018 April 24. The variability characteristics are compared with expectations from standard accretion flow models. Results. We find low variability in total intensity ( σ / μ < 10%), but significantly higher variability in linear and circular polarization (∼30% and ∼50%, respectively). A time-series analysis reveals red-noise variability, with power spectral densities between −2 and −3 across all Stokes parameters. Polarized intensity shows stable intra-day timescales, while total intensity exhibits more variable timescales, suggesting distinct emission regions, with polarization likely arising from a coherent structure. On April 24, a statistically significant inter-band delay in polarized intensity coincides with a near-simultaneous X-ray and millimeter peak that deviates from the typical delayed flare scenario. This event also features enhanced millimeter variability and coherent polarization loop evolution. The observed simultaneity challenges standard models of transient synchrotron emission with cooling delays, favoring instead a scenario of continuous energy injection in an optically thin region. Conclusions. Our results offer new constraints on the physical mechanisms driving variability in Sgr A * , and provide key observational input for refining theoretical models of accretion and plasma behavior in the vicinity of supermassive black holes.

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)0.001
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 score0.004
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.000
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 head0.006
GPT teacher head0.199
Teacher spread0.193 · 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

Citations0
Published2025
Admission routes2
Has abstractyes

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