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Record W4416801361 · doi:10.1051/0004-6361/202557022

Probing jet base emission of M87* with the 2021 Event Horizon Telescope observations

2025· article· en· W4416801361 on OpenAlexaff
Saurabh Kumar, Hendrik Müller, D. Sebastiano von Fellenberg, Paul Tiede, Michaël Janssen, Lindy Blackburn, E. Avery Broderick, Erandi Chavez, Boris Georgiev, P. Thomas Krichbaum, Kotaro Moriyama, Greshma Nair, Iniyan Natarajan, Jongho Park, Andrew West, Maciek Wielgus, Ezequiel Albentosa-Ruíz, 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, Dan Bintley, R. Blundell, Michael Bremer, Roger Brissenden, S. Britzen, Dominique Broguière, Thomas Bronzwaer, Sandra Bustamante, Andrew Chael, Chi‐kwan Chan, Koushik Chatterjee, Shami Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, Xiaopeng Cheng, P. M. Chichura, Ilje Cho, Pierre Christian, Alejandro Cruz-Osorio, Yuzhu Cui, Brandon Curd, Rohan Dahale, Jordy Davelaar, Mariafelicia De Laurentis, Roger Deane, G. Desvignes, Jason Dexter, Vedant Dhruv, Razieh Emami, H. Falcke, Joseph Farah, E. B. Fomalont, H. Alyson Ford, Marianna Foschi, Raquel Fraga-Encinas, Per Friberg, Antonio Fuentes, Peter Galison, Roberto García, Olivier Gentaz, C. Goddi, Roman Gold, Laura Gómez, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, Daryl Haggard, Ronald Hesper, Dirk Heumann, Paul T. P. Ho, Mareki Honma, Lei Huang, Shiro Ikeda, Makoto Inoue, Sara Issaoun, Britton Jeter, Jiang Wu, Alejandra Jiménez-Rosales, Taehyun Jung, R. Karuppusamy, Tomohisa Kawashima, Mark Kettenis, Junhan Kim, Motoki Kino, Jun Yi Koay, Prashant Kocherlakota, Yutaro Kofuji, Shoko Koyama, C. Krämer, 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, Laurent Loinard, Ru-Sen Lu, J. Mao, N. Marchili, Sera Markoff, Iván Martí-Vidal, Satoki Matsushita, Lia Medeiros, Hugo Messias, Izumi Mizuno, Yosuke Mizuno, J. Montgomery, Monika Mościbrodzka, Wanga Mulaudzi, Cornelia Müller, Alejandro Mus, Gibwa Musoke, I. Myserlis, Hiroshi Nagai, Masanori Nakamura, Gopal Narayanan, Antonios Nathanail, Santiago Navarro Fuentes, Joey Neilsen, Chunchong Ni, Hiroki Okino, Héctor Olivares, Tomoaki Oyama, Feryal Özel, Georgios Filippos Paraschos, Harriet Parsons, Nimesh Patel, Ue‐Li Pen, Vincent Piétu, A. V. Plavin, Aleksandar PopStefanija, Oliver Porth, Ben Prather, G. Principe, Dimitrios Psaltis, Hung-Yi Pu, A. Rahlin, Venkatessh Ramakrishnan, Ramprasad Rao, Luciano Rezzolla, Angelo Ricarte, L. Ricci, Bart Ripperda, Jan Röder, Freek Roelofs, Cristina Romero-Cañizales, E. Ros, Arash Roshanineshat, Helge Rottmann, Ignacio Ruiz, Chet Ruszczyk, Salvador Sánchez, David Sánchez-Argüelles, M. Sánchez‐Portal, Mahito Sasada, Kaushik Satapathy, 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, He Sun, Fumie Tazaki, Michael Titus, Kenji Toma, Pablo Torné, Teresa Toscano, Efthalia Traianou, Tyler Trent, Sascha Trippe, Matthew Turk, Ilse van Bemmel, Huib Jan van Langevelde, Jesse Vos, Jan Wagner, D. Ward–Thompson, J. F. C. Wardle, Robert Wharton, K. Wiik, Gunther Witzel, Jompoj Wongphexhauxsorn, Qingwen Wu, Nitika Yadlapalli, Paul Yamaguchi, Aristomenis Yfantis, Doosoo Yoon, André Young, Ziri Younsi, Wei Yu, Feng Yuan, 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
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of LethbridgeCanadian Institute for Advanced ResearchTrinity CollegeMcGill UniversityCanadian Institute for Theoretical AstrophysicsPerimeter InstituteUniversity of WaterlooUniversity of Toronto
Fundersnot available
KeywordsTelescopeJet (fluid)Offset (computer science)Flux (metallurgy)Emission spectrumPosition anglePoint sourceEvent (particle physics)

Abstract

fetched live from OpenAlex

We investigate the presence and spatial characteristics of the jet base emission in M87* at 230 GHz, enabled by the significantly enhanced ( u,v ) coverage in the 2021 Event Horizon Telescope (EHT) observations. The integration of the 12−m Kitt Peak Telescope (USA) and NOEMA (France) stations into the array introduces two critical intermediate-length baselines to SMT (USA) and IRAM 30−m (Spain), providing sensitivity to emission structures at spatial scales of ∼250 μas and ∼2500 μas (∼ 0.02 pc and ∼ 0.02 pc). Without these new baselines, previous EHT observations of the source in 2017 and 2018 lacked the capability to constrain emission on large scales, where a “missing flux” of order ∼1 Jy is expected to reside. To probe these scales, we analyzed closure phases–robust against station-based gain calibration errors–and model the jet base emission using a simple Gaussian component offset from the compact ring emission at spatial separations > 100 μas. Our analysis revealed a Gaussian feature centered at (ΔRA ≈ 320 μas, ΔDec. ≈ 60 μ as), projected separation of ≈ 5500 AU, with an estimated flux density of only ∼60 mJy, implying that most of the missing flux identified in previous EHT studies had to originate from different, larger scales. Brighter emission at the relevant spatial scales is firmly ruled out, and the data do not favor more complex models. This component aligns with the inferred position of the large-scale jet and is therefore physically consistent with the emission of the jet base. While our findings point to detectable jet base emission at 230 GHz, the limited coverage provided by only two intermediate baselines limits our ability to robustly reconstruct its morphology. Consequently, we treated the recovered Gaussian as an upper limit on the jet base flux density. Future EHT observations with expanded intermediate baseline coverage will be essential to constrain the structure and nature of this component with higher precision.

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 score0.003
Threshold uncertainty score0.006

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.007
GPT teacher head0.205
Teacher spread0.197 · 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

Citations2
Published2025
Admission routes1
Has abstractyes

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