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Enregistrement W3015473161 · doi:10.1051/0004-6361/202037493

Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

2020· article· en· W3015473161 sur OpenAlexafffund
Jae-Young Kim, T. P. Krichbaum, Avery E. Broderick, Maciek Wielgus, Lindy Blackburn, José L. Gómez, Michael D. Johnson, Katherine L. Bouman, Andrew Chael, Kazunori Akiyama, Svetlana G. Jorstad, Alan P. Marscher, Sara Issaoun, Michaël Janssen, Chi‐kwan Chan, T. Savolainen, Dominic W. Pesce, Feryal Özel, W. Alef, Keiichi Asada, Rebecca Azulay, Anne-Kathrin Baczko, David Ball, Mislav Baloković, John Barrett, Dan Bintley, W. Boland, Geoffrey C. Bower, Michael Bremer, Christiaan D. Brinkerink, Roger Brissenden, S. Britzen, Dominique Broguière, Thomas Bronzwaer, Do‐Young Byun, J. E. Carlstrom, Shami Chatterjee, Koushik Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, Ilje Cho, Pierre Christian, J. E. Conway, J. M. Cordes, G. Crew, Yuzhu Cui, Jordy Davelaar, Mariafelicia De Laurentis, Roger Deane, Jessica Dempsey, G. Desvignes, Jason Dexter, Sheperd S. Doeleman, Ralph P. Eatough, H. Falcke, Vincent L. Fish, Ed Fomalont, Raquel Fraga-Encinas, Per Friberg, Christian M. Fromm, Peter Galison, Charles F. Gammie, Roberto García, Olivier Gentaz, Boris Georgiev, C. Goddi, Roman Gold, Arturo I. Gómez-Ruiz, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, M. H. Hecht, Ronald Hesper, Luis C. Ho, Paul T. P. Ho, Mareki Honma, Lei Huang, D. H. Hughes, Shiro Ikeda, Makoto Inoue, D. J. James, Buell T. Jannuzi, Britton Jeter, Alejandra Jiménez-Rosales, Taehyun Jung, Mansour Karami, R. Karuppusamy, Tomohisa Kawashima, Garrett K. Keating, Mark Kettenis, Junhan Kim, Jongsoo Kim, Motoki Kino, Jun Yi Koay, Patrick M. Koch, Shoko Koyama, C. Krämer, Cheng‐Yu Kuo, Tod R. Lauer, Sang-Sung Lee, Yanrong Li, M. Lindqvist, Rocco Lico, Kuo Liu, Elisabetta Liuzzo, Wen-Ping Lo, A. P. Lobanov, Laurent Loinard, C. J. Lonsdale, Ru-Sen Lu, Nicholas R. MacDonald, Jirong Mao, Sera Markoff, Daniel P. Marrone, I. Martí‐Vidal, Satoki Matsushita, Lynn D. Matthews, Lia Medeiros, K. M. Menten, Yosuke Mizuno, Izumi Mizuno, J. M. Moran, Kotaro Moriyama, Monika Mościbrodzka, Gibwa Musoke, Cornelia Müller, Hiroshi Nagai, Neil M. Nagar, Masanori Nakamura, Ramesh Narayan, Gopal Narayanan, Iniyan Natarajan, R. Neri, Chunchong Ni, A. Noutsos, Hiroki Okino, Héctor Olivares, Gisela N. Ortiz-León, Tomoaki Oyama, Daniel C. M. Palumbo, Jongho Park, Nimesh Patel, Ue‐Li Pen, Vincent Piétu, R. L. Plambeck, Aleksandar PopStefanija, Oliver Porth, Ben Prather, Jorge A. Preciado-López, Dimitrios Psaltis, Hung-Yi Pu, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Alexander W. Raymond, Luciano Rezzolla, Bart Ripperda, Freek Roelofs, A. E. E. Rogers, E. Ros, Mel Rose, Arash Roshanineshat, H. Rottmann, A. L. Roy, Benjamin R. Ryan, K. L. J. Rygl, Salvador Sánchez, David Sánchez-Argüelles, Mahito Sasada, F. Peter Schloerb, K. Schüster, Lijing Shao, Zhi-Qiang Shen, Des Small, Bong Won Sohn, Jason Soohoo, Fumie Tazaki, Paul Tiede, R. P. J. Tilanus, Michael S. Titus, Kenji Toma, Pablo Torné, Tyler Trent, Efthalia Traianou, Sascha Trippe, Shuichiro Tsuda, Ilse van Bemmel, Huib Jan van Langevelde, Daniel R. van Rossum, Jan Wagner, J. F. C. Wardle, D. Ward–Thompson, Jonathan Weintroub, Norbert Wex, Robert Wharton, George N. Wong, Qingwen Wu, Doosoo Yoon, André Young, Ken Young, Ziri Younsi, Ye‐Fei Yuan, Ye‐Fei Yuan, J. A. Zensus, Guang-Yao Zhao, Shan-Shan Zhao, Ziyan Zhu, Juan Carlos Algaba, Alexander Allardi, Rodrigo Amestica, J. Anczarski, U. Bach, Frederick K. Baganoff, Christopher Beaudoin, B. A. Benson, Ryan Berthold, J. Blanchard, R. Blundell, Sandra Bustamente, R. J. Cappallo, Edgar Castillo-Domínguez, Chih-Cheng Chang, Shu-Hao Chang, Song-Chu Chang, Chung-Chen Chen, Ryan Chilson, Tim C. Chuter, Rodrigo Córdova Rosado, I. M. Coulson, Joseph Crowley, M. Derome, Matthew R. Dexter, Sven Dornbusch, Kevin A. Dudevoir, Sergio A. Dzib, Andreas Eckart, Chris Eckert, N. R. Erickson, W. Everett, Aaron Faber, Joseph Farah, Vernon Fath, Thomas W. Folkers, David C. Forbes, R. Freund, David M. Gale, F. Gao, Gertie Geertsema, D. A. Graham, Christopher H. Greer, Ronald Grosslein, Frédéric Gueth, Daryl Haggard, N. W. Halverson, Chih-Chiang Han, Kuo-Chang Han, H. Jinchi, Yutaka Hasegawa, J. W. Henning, A. Hernández-Gómez, R. Herrero‐Illana, S. Heyminck, Akihiko Hirota, James Hoge, Yau-De Huang, C. M. Violette Impellizzeri, Homin Jiang, John David, A. Kamble, Ryan Keisler, Kimihiro Kimura, Yusuke Kono, Derek Kubo, John Kuroda, Richard Lacasse, Robert A. Laing, E. M. Leitch, Chao-Te Li, L. C.-C. Lin, Ching-Tang Liu, Kuan-Yu Liu, Li-Ming Lu, R. G. Marson, Pierre Martin-Cocher, Kyle Massingill, Callie Matulonis, Martin P. McColl, Stephen R. McWhirter, Hugo Messias, Zheng Meyer-Zhao, Daniel Michalik, Alfredo Montaña, William Montgomerie, Matias Mora-Klein, D. Muders, Andrew Nadolski, S. Navarro, Joey Neilsen, Chi H. Nguyen, Hiroaki Nishioka, Timothy Norton, Michael A. Nowak, George Nystrom, Hideo Ogawa, Peter Oshiro, Tomoaki Oyama, Harriet Parsons, J. Peñalver, N. Phillips, Michael Poirier, Nicolas Pradel, Rurik A. Primiani, Philippe Raffin, A. Rahlin, George Reiland, C. Risacher, Ignacio Ruiz, Alejandro F. Sáez-Madaín, Remi Sassella, P. Schellart, Paul Shaw, Kevin M. Silva, Hotaka Shiokawa, David R. Smith, W. M. Snow, Kamal Souccar, Don Sousa, T. K. Sridharan, Ranjani Srinivasan, William Stahm, A. A. Stark, Kyle Story, Sjoerd T. Timmer, Laura Vertatschitsch, Craig Walther, Tashun Wei, N. Whitehorn, A. R. Whitney, D. P. Woody, J. G. A. Wouterloot, Melvin Wright, Paul Yamaguchi, Chen-Yu Yu, M. Zeballos, Shuo Zhang, L. M. Ziurys

Notice bibliographique

RevueAstronomy and Astrophysics · 2020
Typearticle
Langueen
DomainePhysics and Astronomy
ThématiqueAstrophysics and Cosmic Phenomena
Établissements canadiensMcGill UniversityWestern UniversityCanadian Institute for Theoretical AstrophysicsCanadian Institute for Advanced ResearchUniversity of TorontoPerimeter InstituteUniversity of Waterloo
Organismes subventionnairesLos Alamos National LaboratoryOffice of International Science and EngineeringNational Key Research and Development Program of ChinaComisión Nacional de Investigación Científica y TecnológicaJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNational Nuclear Security AdministrationInstitut Périmètre de physique théoriqueRecruitment Program of Global ExpertsAcademy of FinlandMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueNational Natural Science Foundation of ChinaNational Research Foundation of KoreaMinisterio de Ciencia, Innovación y UniversidadesNuclear Safety and Security CommissionGeneralitat ValencianaNatural Sciences and Engineering Research Council of CanadaChina Scholarship CouncilEuropean Southern ObservatoryMinistry of Education, Culture, Sports, Science and TechnologyJohn Templeton FoundationMinisterio de Economía y CompetitividadNederlandse Organisatie voor Wetenschappelijk OnderzoekInstituto de Astrofísica de AndalucíaChinese Academy of SciencesAcademia SinicaVetenskapsrådetInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologySmithsonian InstitutionU.S. Department of EnergyKavli FoundationEuropean CommissionLeverhulme TrustNational Radio Astronomy ObservatoryHarvard UniversityToray Science FoundationNational Research FoundationUniversity of ArizonaUniversidad Nacional Autónoma de MéxicoKorea Astronomy and Space Science InstituteAssociated UniversitiesSpace Telescope Science InstituteNational Science FoundationCompute CanadaNational Astronomical Observatory of JapanDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaUniversity of ChicagoNational Institutes of Natural SciencesGovernment of CanadaNational Aeronautics and Space AdministrationIstituto Nazionale di Fisica NucleareDepartment of Science and Technology, Ministry of Science and Technology, IndiaRussian Science FoundationGordon and Betty Moore Foundation
Mots-clésPhysicsBlazarAstrophysicsAstronomyEvent (particle physics)TelescopeQuasarGamma rayGalaxy

Résumé

récupéré en direct d'OpenAlex

3C 279 is an archetypal blazar with a prominent radio jet that show broadband flux density variability across the entire electromagnetic spectrum. We use an ultra-high angular resolution technique – global Very Long Baseline Interferometry (VLBI) at 1.3 mm (230 GHz) – to resolve the innermost jet of 3C 279 in order to study its fine-scale morphology close to the jet base where highly variable γ -ray emission is thought to originate, according to various models. The source was observed during four days in April 2017 with the Event Horizon Telescope at 230 GHz, including the phased Atacama Large Millimeter/submillimeter Array (ALMA), at an angular resolution of ∼20 μ as (at a redshift of z = 0.536 this corresponds to ∼0.13 pc ∼ 1700 Schwarzschild radii with a black hole mass M BH = 8 × 10 8 M ⊙ ). Imaging and model-fitting techniques were applied to the data to parameterize the fine-scale source structure and its variation. We find a multicomponent inner jet morphology with the northernmost component elongated perpendicular to the direction of the jet, as imaged at longer wavelengths. The elongated nuclear structure is consistent on all four observing days and across different imaging methods and model-fitting techniques, and therefore appears robust. Owing to its compactness and brightness, we associate the northern nuclear structure as the VLBI “core”. This morphology can be interpreted as either a broad resolved jet base or a spatially bent jet. We also find significant day-to-day variations in the closure phases, which appear most pronounced on the triangles with the longest baselines. Our analysis shows that this variation is related to a systematic change of the source structure. Two inner jet components move non-radially at apparent speeds of ∼15 c and ∼20 c (∼1.3 and ∼1.7 μ as day −1 , respectively), which more strongly supports the scenario of traveling shocks or instabilities in a bent, possibly rotating jet. The observed apparent speeds are also coincident with the 3C 279 large-scale jet kinematics observed at longer (cm) wavelengths, suggesting no significant jet acceleration between the 1.3 mm core and the outer jet. The intrinsic brightness temperature of the jet components are ≲10 10 K, a magnitude or more lower than typical values seen at ≥7 mm wavelengths. The low brightness temperature and morphological complexity suggest that the core region of 3C 279 becomes optically thin at short (mm) wavelengths.

Récupéré en direct depuis OpenAlex et désinversé. Les résumés ne sont pas conservés dans cette base de données : les index inversés représentent 8,6 Go des 9,3 Go de texte de la base, et le serveur dispose de 13 Go libres.

Comment cette classification a été obtenuedéplier

Prédiction distillée sur la base complète

Imitation des enseignants

Ni prévalence calibrée, ni vérité terrain. Validation humaine à venir. Apprise à partir de 10 348 étiquettes directes de Codex et de 10 348 étiquettes directes de Gemma. Le mode candidate est l'union des têtes enseignantes seuillées; le consensus est leur intersection. Ces sorties portent le statut machine_predicted_unvalidated et ne sont ni des étiquettes humaines ni des étiquettes directes de modèles de pointe.

score de la tête « metaresearch » (Codex)0,000
score de la tête « metaresearch » (Gemma)0,000
Version: codex-gemma-dda1882f352aStatut de validation: machine_predicted_unvalidated
Catégories candidatesMéta-épidémiologie (sens strict)
Catégories consensuellesaucune
DomaineSignal candidat: aucune · Signal consensuel: aucune
Devis d'étudeSignal candidat: Autre devis · Signal consensuel: aucune
GenreSignal candidat: Empirique · Signal consensuel: Empirique
Score de désaccord entre enseignants0,791
Score d'incertitude au seuil1,000

Scores Codex et Gemma par catégorie

CatégorieCodexGemma
Métarecherche0,0000,000
Méta-épidémiologie (sens strict)0,0000,000
Méta-épidémiologie (sens large)0,0000,000
Bibliométrie0,0000,000
Études des sciences et des technologies0,0000,000
Communication savante0,0000,000
Science ouverte0,0000,000
Intégrité de la recherche0,0000,000
Charge utile insuffisante (le modèle a refusé de juger)0,0000,000

Scores machine (provisoires)

Les deux têtes enseignantes du modèle étudiant, lues sur ce travail. Un score ordonne la base pour la relecture; il n'affirme jamais une catégorie, et le statut de validation accompagne chaque rangée tel quel.

Scores de référence d'un modèle non mature (critères de maturité non atteints, 7 itérations). Un score ordonne; il n'affirme jamais une catégorie.

Tête enseignante Opus0,012
Tête enseignante GPT0,201
Écart entre enseignants0,189 · la distance entre les deux têtes enseignantes sur ce seul travail
Statut de validationscore_only:v0-immature-baseline · tel quel depuis la passe de notation : score_only signifie que le nombre peut ordonner les travaux, et qu'aucune étiquette de catégorie n'en découle

Classification

machine, non validée

Prédiction automatique; un appel candidat d’une seule tête enseignante, pas un consensus.

Devis d'étudeAutre devis
Domainenon disponible
GenreEmpirique

Le détail, modèle par modèle et score par score, se trouve en fin de page sous « Comment cette classification a été obtenue ».

En bref

Citations105
Publié2020
Routes d'admission2
Résumé présentoui

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