First M87 Event Horizon Telescope Results. II. Array and Instrumentation
Abstract
Abstract The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ∼1.3 mm, EHT angular resolution ( λ / D ) is ∼25 μ as, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64 gigabit s −1 , exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate in M87.
Funding
- National Science Foundation
- Smithsonian Institution
- U.S. Department of Energy
- National Aeronautics and Space Administration
- John Templeton Foundation
- Gordon and Betty Moore Foundation
- Massachusetts Institute of Technology
- Harvard University
- University of Chicago
- University of Arizona
- Innovation, Science and Economic Development Canada
- Compute Canada
- Strong
- Ministerio de Ciencia, Innovación y Universidades
- National Radio Astronomy Observatory
- Associated Universities
- International Max Planck Research School for Environmental, Cellular and Molecular Microbiology
- Government of Canada
- Leverhulme Trust
- European Commission
- National Research Foundation
- Department of Science and Technology, Ministry of Science and Technology, India
- Ministry of Education, Culture, Sports, Science and Technology
- Academia Sinica
- Chinese Academy of Sciences
- Consejo Nacional de Ciencia y Tecnología
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek
- Ministerio de Economía y Competitividad
- Generalitat Valenciana
- Korea Astronomy and Space Science Institute
- National Research Foundation of Korea
- Max-Planck-Gesellschaft
- Vetenskapsrådet
- China Scholarship Council
- European Southern Observatory
- Centre National de la Recherche Scientifique
- Universidad Nacional Autónoma de México
- National Astronomical Observatory of Japan
- Russian Science Foundation
- Ministero dello Sviluppo Economico
- Recruitment Program of Global Experts
- Istituto Nazionale di Fisica Nucleare
- Instituto de Astrofísica de Andalucía
- Institut Périmètre de physique théorique
- Toray Science Foundation
- National Nuclear Security Administration
- Natural Sciences and Engineering Research Council of Canada
- Japan Society for the Promotion of Science
- Comisión Nacional de Investigación Científica y Tecnológica
- Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
- National Institutes of Natural Sciences
- Office of Polar Programs
- Los Alamos National Laboratory
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