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Record W4410460359 · doi:10.1051/0004-6361/202554140

First polarization study of the M87 jet and active galactic nuclei at submillimeter wavelengths with ALMA

2025· article· en· W4410460359 on OpenAlexfundno aff
C. Goddi, G. Crew, Lynn D. Matthews, Hugo Messias, Alejandro Mus, Iván Martí-Vidal, Ezequiel Albentosa-Ruíz, Mariafelicia De Laurentis, Elisabetta Liuzzo, N. Marchili, L.J. Kazi Rygl, 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, 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, Koushik Chatterjee, Shami Chatterjee, Ming‐Tang Chen, T. M. Crawford, Brandon Curd, Rohan Dahale, Jessica Dempsey, Ralph P. Eatough, Joseph Farah, H. Alyson Ford, Marianna Foschi, Raquel Fraga-Encinas, William T. Freeman, Roberto García, Mark Gurwell, D. H. Hughes, 何子山, Shiro Ikeda, Sara Issaoun, Svetlana G. Jorstad, Abhishek V. Joshi, Junhan Kim, Motoki Kino, Yutaro Kofuji, T. P. Krichbaum, Aviad Levis, Zhiyuan Li, Rocco Lico, M. Lindqvist, Wen-Ping Lo, Ru-Sen Lu, K. M. Menten, Yosuke Mizuno, 毛基荣, Monika Mościbrodzka, Cornelia Müller, I. Myserlis, Masanori Nakamura, Michael A. Nowak, Hiroki Okino, Daniel C. M. Palumbo, Jongho Park, Harriet Parsons, Nimesh Patel, V. Piétu, Oliver Porth, Venkatessh Ramakrishnan, Freek Roelofs, E. Ros, David Sánchez-Argüelles, Mahito Sasada, Kaushik Satapathy, F. Peter Schloerb, Jonathan Schonfeld, K. Schüster, S. Silpa, Jason Soohoo, Joshua S. Stanway, Alexandra J. Tetarenko, Kenji Toma, Pablo Torné, Tyler Trent, Matthew Turk, Ilse van Bemmel, Michael F. Wondrak, Qingwen Wu, Nitika Yadlapalli, Paul Yamaguchi, Aristomenis Yfantis, Doosoo Yoon, André Young, Ziri Younsi, Wei Yu, J. A. Zensus, Shuo Zhang, Guang-Yao Zhao, Shan-Shan Zhao

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersLos Alamos National LaboratoryOak Ridge National LaboratoryHigh Energy PhysicsNational Key Research and Development Program of ChinaAgencia Estatal de InvestigaciónFundação para a Ciência e a TecnologiaJapan Society for the Promotion of ScienceHORIZON EUROPE Framework ProgrammeNational Nuclear Security AdministrationOffice of ScienceToray Science FoundationEast Asian Core Observatories AssociationInstitut Périmètre de physique théoriqueAlliance de recherche numérique du CanadaNational Science and Technology CouncilAgencia Nacional de Investigación y DesarrolloFundación Bancaria Caixa d'Estalvis i Pensions de BarcelonaMinistry of Science and ICT, South KoreaIstituto Nazionale di Fisica NucleareUniversiteit van AmsterdamJunta de AndalucíaNational Astronomical Observatory of JapanShanghai Jiao Tong UniversityCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftNational Natural Science Foundation of ChinaNational Research Foundation of KoreaGeneralitat ValencianaNational Science FoundationChina Postdoctoral Science FoundationInstituto de Astrofísica de AndalucíaDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekChinese Academy of SciencesAcademia SinicaUniversidad Nacional Autónoma de MéxicoCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorEuropean CommissionLeverhulme TrustNational Radio Astronomy ObservatoryFundação de Amparo à Pesquisa do Estado de São PauloCanada Research ChairsNetherlands eScience CenterJohn Templeton FoundationChina Scholarship CouncilMinistry of Education, Culture, Sports, Science and TechnologyRadboud UniversiteitNational Research FoundationUniversity of PretoriaJoint Institute for Computational Fundamental ScienceUniversity of ArizonaSmithsonian InstitutionInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyFonds de recherche du Québec – Nature et technologiesVetenskapsrådetU.S. Department of EnergyConsejo Superior de Investigaciones CientíficasUniversity of ChicagoNational Institutes of Natural SciencesGovernment of CanadaMinisterio de Ciencia, Innovación y UniversidadesGordon and Betty Moore FoundationCERNNational 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
KeywordsPhysicsAstrophysicsActive galactic nucleusPolarization (electrochemistry)AstronomyWavelengthSubmillimeter ArrayGalaxyStar formationOptics

Abstract

fetched live from OpenAlex

Aims. We investigated the polarization and Faraday properties of Messier 87 (M87) and seven other radio-loud active galactic nuclei (AGNs) at λ 0.87 mm (345 GHz) using the Atacama Large Millimeter/submillimeter Array (ALMA). Our goal was to characterize the linear polarization (LP) fractions, measure Faraday rotation measures (RMs), and examine the magnetic field structures in the emission regions of these AGNs. Methods. We conducted full-polarization observations as part of the ALMA Band 7 very long baseline interferometry (VLBI) commissioning during the April 2021 Event Horizon Telescope (EHT) campaign. We analyzed the LP fractions and RMs to assess the nature of Faraday screens and magnetic fields in the submillimeter emission regions. Results. We find LP fractions between 1% and 17% and RMs exceeding 10 5 rad m −2 , which are 1–2 orders of magnitude higher than typically observed at longer wavelengths ( λ >3 mm). This suggests denser Faraday screens or stronger magnetic fields. Additionally, we present the first submillimeter polarized images of the M87 jet and the observed AGNs, revealing RM gradients and sign reversals in the M87 jet indicative of a kiloparsec-scale helical magnetic field structure. Conclusions. Our results provide essential constraints for calibrating, analyzing, and interpreting VLBI data from the EHT at 345 GHz, representing a critical step toward submillimeter VLBI imaging.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.242
Threshold uncertainty score0.804

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 science0.0000.000
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 head0.004
GPT teacher head0.188
Teacher spread0.184 · 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 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

Citations7
Published2025
Admission routes1
Has abstractyes

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