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Record W3123227886 · doi:10.1051/0004-6361/201936622

SYMBA: An end-to-end VLBI synthetic data generation pipeline

2019· article· en· W3123227886 on OpenAlexafffund
Freek Roelofs, Michaël Janssen, Iniyan Natarajan, Roger Deane, Jordy Davelaar, Héctor Olivares, Oliver Porth, Scott Paine, Katherine L. Bouman, R. P. J. Tilanus, Ilse van Bemmel, H. Falcke, Kazunori Akiyama, A. Alberdi, W. Alef, Keiichi Asada, Rebecca Azulay, Anne-Kathrin Baczko, D. R. Ball, Mislav Baloković, John Barrett, Dan Bintley, Lindy Blackburn, W. Boland, Geoffrey C. Bower, Michael Bremer, Christiaan D. Brinkerink, Roger Brissenden, S. Britzen, Avery E. Broderick, Dominique Broguière, Thomas Bronzwaer, Do‐Young Byun, J. E. Carlstrom, Andrew Chael, Chi‐kwan Chan, Shami Chatterjee, Koushik Chatterjee, Ming‐Tang Chen, Y. Chen, Ilje Cho, Pierre Christian, J. E. Conway, J. M. Cordes, G. Crew, Yuzhu Cui, Mariafelicia De Laurentis, Jessica Dempsey, G. Desvignes, Jason Dexter, Sheperd S. Doeleman, Ralph P. Eatough, Vincent L. Fish, E. B. Fomalont, Raquel Fraga-Encinas, Per Friberg, Christian M. Fromm, José L. Gómez, Peter Galison, Charles F. Gammie, Roberto García, Olivier Gentaz, Boris Georgiev, C. Goddi, Roman Gold, 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, Sara Issaoun, D. J. James, Buell T. Jannuzi, Britton Jeter, Michael D. Johnson, Svetlana G. Jorstad, Taehyun Jung, Mansour Karami, R. Karuppusamy, Tomohisa Kawashima, Garrett K. Keating, Mark Kettenis, Jae-Young Kim, J. Kim, M. Kino, Jun Yi Koay, Patrick M. Koch, Shoko Koyama, C. Krämer, T. P. Krichbaum, Cheng‐Yu Kuo, Tod R. Lauer, S. Lee, Y. 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, J. Mao, Sera Markoff, Daniel P. Marrone, A. P. Marscher, I. Martí‐Vidal, Satoki Matsushita, Lynn D. Matthews, Lia Medeiros, K. M. Menten, Yosuke Mizuno, Izumi Mizuno, J. M. Moran, Kotaro Moriyama, Monika Mościbrodzka, C. Müller, Hiroshi Nagai, Neil M. Nagar, Makoto Nakamura, Ramesh Narayan, Gopal Narayanan, R. Neri, Chunchong Ni, A. Noutsos, Hiroki Okino, H. Olivares, Gisela N. Ortiz-León, Tomoaki Oyama, Feryal Özel, Daniel C. M. Palumbo, Nimesh Patel, Ue‐Li Pen, Dominic W. Pesce, V. Piétu, R. Plambeck, Aleksandar PopStefanija, Ben Prather, Jorge A. Preciado-López, D. Psaltis, Hung-Yi Pu, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Alexander W. Raymond, L. Rezzolla, Bart Ripperda, A. E. E. Rogers, E. Ros, Mel Rose, A. Roshanineshat, H. Rottmann, C. Ruszczyk, B. R. Ryan, K. L. J. Rygl, S. Sánchez, David Sánchez-Argüelles, Mahito Sasada, T. Savolainen, F. Peter Schloerb, K. Schüster, Lijing Shao, Z. Shen, Des Small, Bong Won Sohn, Jason Soohoo, Fumie Tazaki, Paul Tiede, Michael Titus, Kenji Toma, Pablo Torné, Efthalia Traianou, T. Trent, Sascha Trippe, S. Tsuda, Huib Jan van Langevelde, Daniel R. van Rossum, Jan Wagner, J. F. C. Wardle, Jonathan Weintroub, N. Wex, Robert Wharton, Maciek Wielgus, George N. Wong, Q. Wu, André Young, Kenneth H. Young, Ziri Younsi, F. Yuan, Y. Yuan, J. A. Zensus, Guang-Yao Zhao, Shan-Shan Zhao, Ziyan Zhu

Bibliographic record

VenueAstronomy and Astrophysics · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsCanadian Institute for Theoretical AstrophysicsCanadian Institute for Advanced ResearchUniversity of TorontoPerimeter InstituteUniversity of Waterloo
FundersLos 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 ScienceChina Scholarship CouncilEuropean Southern ObservatoryMinistry of Education, Culture, Sports, Science and TechnologyJohn Templeton FoundationMinisterio de Economía y CompetitividadNatural Sciences and Engineering Research Council of CanadaNational 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 ValencianaDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaNederlandse Organisatie voor Wetenschappelijk OnderzoekInstituto de Astrofísica de AndalucíaChinese Academy of SciencesVetenskapsrådetInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologySmithsonian InstitutionU.S. Department of EnergyEuropean CommissionLeverhulme TrustNational Radio Astronomy ObservatoryHarvard UniversityToray Science FoundationNational Research FoundationUniversity of ArizonaNational Astronomical Observatory of JapanSpace Telescope Science InstituteAssociated UniversitiesUniversidad Nacional Autónoma de MéxicoKorea Astronomy and Space Science InstituteNational Science FoundationCompute CanadaNational Institutes of Natural SciencesGovernment of CanadaIstituto Nazionale di Fisica NucleareDepartment of Science and Technology, Ministry of Science and Technology, IndiaRussian Science FoundationGordon and Betty Moore FoundationNational Aeronautics and Space AdministrationAcademia SinicaFlatiron Health
KeywordsPhysicsVery-long-baseline interferometryAstrophysicsAstronomyEnd-to-end principle

Abstract

fetched live from OpenAlex

Context. Realistic synthetic observations of theoretical source models are essential for our understanding of real observational data. In using synthetic data, one can verify the extent to which source parameters can be recovered and evaluate how various data corruption effects can be calibrated. These studies are the most important when proposing observations of new sources, in the characterization of the capabilities of new or upgraded instruments, and when verifying model-based theoretical predictions in a direct comparison with observational data. Aims. We present the SYnthetic Measurement creator for long Baseline Arrays ( SYMBA ), a novel synthetic data generation pipeline for Very Long Baseline Interferometry (VLBI) observations. SYMBA takes into account several realistic atmospheric, instrumental, and calibration effects. Methods. We used SYMBA to create synthetic observations for the Event Horizon Telescope (EHT), a millimetre VLBI array, which has recently captured the first image of a black hole shadow. After testing SYMBA with simple source and corruption models, we study the importance of including all corruption and calibration effects, compared to the addition of thermal noise only. Using synthetic data based on two example general relativistic magnetohydrodynamics (GRMHD) model images of M 87, we performed case studies to assess the image quality that can be obtained with the current and future EHT array for different weather conditions. Results. Our synthetic observations show that the effects of atmospheric and instrumental corruptions on the measured visibilities are significant. Despite these effects, we demonstrate how the overall structure of our GRMHD source models can be recovered robustly with the EHT2017 array after performing calibration steps, which include fringe fitting, a priori amplitude and network calibration, and self-calibration. With the planned addition of new stations to the EHT array in the coming years, images could be reconstructed with higher angular resolution and dynamic range. In our case study, these improvements allowed for a distinction between a thermal and a non-thermal GRMHD model based on salient features in reconstructed images.

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 score0.932
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 communication0.0000.001
Open science0.0010.000
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 head0.019
GPT teacher head0.235
Teacher spread0.215 · 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".

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Citations36
Published2019
Admission routes2
Has abstractyes

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