MétaCan
Menu
Back to cohort
Record W4414195689 · doi:10.1051/0004-6361/202555855

Horizon-scale variability of M87* from 2017–2021 EHT observations

2025· article· en· W4414195689 on OpenAlexaff
Kazunori Akiyama, Ezequiel Albentosa-Ruíz, 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, Erandi Chavez, Koushik Chatterjee, Shami Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, P. M. Chichura, Ilje Cho, Pierre Christian, 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, G. Desvignes, Jason Dexter, Vedant Dhruv, 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, Raquel Fraga-Encinas, Per Friberg, Antonio Fuentes, Peter Galison, Charles F. Gammie, Roberto García, Olivier Gentaz, Boris Georgiev, C. Goddi, Roman Gold, I. Arturo Gómez-Ruiz, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, Daryl Haggard, Ronald Hesper, Dirk Heumann, Paul T. P. Ho, Dan Hoak, Mareki Honma, Lei 磊 Huang 黄, 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, C. Adam Jones, Taehyun Jung, R. Karuppusamy, Tomohisa Kawashima, Katie M. Keating, Mark Kettenis, Dong-Jin Kim, Jae-Young 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, Deokhyeong Lee, Sang-Sung Lee, Aviad Levis, Zhiyuan 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, N. Marchili, Sera Markoff, Daniel P. Marrone, Alan P. Marscher, Iván Martí-Vidal, Satoki Matsushita, Lia Medeiros, M. Karl Menten, Izumi Mizuno, Yosuke Mizuno, J. Montgomery, Michael E. Moran, Kotaro Moriyama, Monika Mościbrodzka, Wanga Mulaudzi, Cornelia Müller, Hendrik Müller, Alejandro Mus, Gibwa Musoke, 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, A. V. Plavin, Aleksandar PopStefanija, Oliver Porth, Ben Prather, G. Principe, Dimitrios Psaltis, Hung-Yi Pu, A. Rahlin, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Luciano Rezzolla, Angelo Ricarte, L. Ricci, Bart Ripperda, Jan Röder, Freek Roelofs, Cristina Romero-Cañizales, E. Ros, Arash Roshanineshat, H. Rottmann, Ignacio Ruiz, C. Ruszczyk, L.J. Kazi Rygl, D.S. León Salas, Salvador Sánchez, David Sánchez-Argüelles, M. 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, Randall W. Smith, Bong Won Sohn, Jason Soohoo, Kamal Souccar, Joshua S. Stanway, Fumie Tazaki, Alexandra J. Tetarenko, Paul Tiede, R. P. J. Tilanus, 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, D. Sebastiano von Fellenberg, Jesse Vos, Jan Wagner, D. Ward–Thompson, J. F. C. Wardle, E. Washington, Robert Wharton, Maciek Wielgus, K. Wiik, Gunther Witzel, Jompoj Wongphexhauxsorn, Qingwen Wu, Nitika Yadlapalli, Paul Yamaguchi, Aristomenis Yfantis, Doosoo Yoon, André Young, Ziri Younsi, Ai-Ling Zeng, J. A. Zensus, Shuo Zhang, Guang-Yao Zhao, Shan-Shan Zhao, Ryan Berthold, Shu-Hao Chang, Ryan Chilson, Chih-Chiang Han, Gertie Geertsema, José Luis Hernández-Rebollar, Teddy Huang, Derek Kubo, Daniel Michalik, Alfredo Montaña, Andrew Nadolski, Peter Oshiro, Iván Rodríguez-Montoya, Tashun Wei

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of LethbridgeCanadian Institute for Theoretical AstrophysicsCanadian Institute for Advanced ResearchTrinity CollegeMcGill UniversityUniversity of TorontoPerimeter InstituteUniversity of Waterloo
Fundersnot available
KeywordsPosition angleLinear polarizationVery Long Baseline ArrayVery-long-baseline interferometryTelescopeSupermassive black holePolarization (electrochemistry)BrightnessAccretion (finance)

Abstract

fetched live from OpenAlex

We report three epochs of polarized images of M87* at 230 GHz using data from the Event Horizon Telescope (EHT) taken in 2017, 2018, and 2021. The baseline coverage of the 2021 observations is significantly improved through the addition of two new EHT stations: the 12 m Kitt Peak Telescope and the Northern Extended Millimetre Array (NOEMA). All observations result in images dominated by a bright, asymmetric ring with a persistent diameter of 43.9 ± 0.6 μas, consistent with expectations for lensed synchrotron emission encircling the apparent shadow of a supermassive black hole. We find that the total intensity and linear polarization of M87* vary significantly across the three epochs. Specifically, the azimuthal brightness distribution of the total intensity images varies from year to year, as expected for a stochastic accretion flow. However, despite a gamma-ray flare erupting in M87 quasi-contemporaneously to the 2018 observations, the 2018 and 2021 images look remarkably similar. The resolved linear polarization fractions in 2018 and 2021 peak at ∼5%, compared to ∼15% in 2017. The spiral polarization pattern on the ring also varies from year to year, including a change in the electric vector position angle helicity in 2021 that could reflect changes in the magnetized accretion flow or an external Faraday screen. The improved 2021 coverage also provides the first EHT constraints on jet emission outside the ring, on scales of ≲1 mas. Overall, these observations provide strong proof of the reliability of the EHT images and probe the dynamic properties of the horizon-scale accretion flow surrounding M87*.

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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.738
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 studies0.0000.000
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 head0.008
GPT teacher head0.209
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.

Study designOther design
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

Citations10
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueAstronomy and AstrophysicsSame topicAstrophysics and Cosmic PhenomenaFrench-language works237,207