First M87 Event Horizon Telescope Results. II. Array and Instrumentation
Artikel i vetenskaplig tidskrift, 2019
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 μas, 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.
Visa mer
gravitational lensing: strong
black hole physics
techniques: high angular resolution
instrumentation: interferometers
galaxies: individual (M87)
Galaxy: center
Författare
Kazunori Akiyama
National Astronomical Observatory of Japan
Harvard University
National Radio Astronomy Observatory
Massachusetts Institute of Technology (MIT)
Antxon Alberdi
Consejo Superior de Investigaciones Científicas (CSIC)
Walter Alef
Max-Planck-Gesellschaft
K. Asada
National Taiwan University
R. Azulay
Max-Planck-Gesellschaft
Universitat de Valencia
A. K. Baczko
Max-Planck-Gesellschaft
David Ball
University of Arizona
Mislav Baloković
Harvard University
Harvard-Smithsonian Center for Astrophysics
John Barrett
Massachusetts Institute of Technology (MIT)
Dan Bintley
East Asian Observatory
Lindy Blackburn
Harvard University
Harvard-Smithsonian Center for Astrophysics
W. Boland
Nederlandse Onderzoekschool voor Astronomie (NOVA)
K. L. Bouman
Harvard University
Harvard-Smithsonian Center for Astrophysics
California Institute of Technology (Caltech)
G. C. Bower
Academia Sinica
M. Bremer
Institut de Radioastronomie Millimétrique (IRAM)
C. D. Brinkerink
Radboud Universiteit
Roger Brissenden
Harvard University
Harvard-Smithsonian Center for Astrophysics
Silke Britzen
Max-Planck-Gesellschaft
Avery E. Broderick
Perimeter Institute for Theoretical Physics
University of Waterloo
D. Broguière
Institut de Radioastronomie Millimétrique (IRAM)
Thomas Bronzwaer
Radboud Universiteit
Do Young Byun
University of Science and Technology (UST)
Korea Astronomy and Space Science Institute
J. E. Carlstrom
University of Chicago
A. Chael
Harvard University
Harvard-Smithsonian Center for Astrophysics
Chi Kwan Chan
University of Arizona
S. Chatterjee
Cornell University
Koushik Chatterjee
Universiteit Van Amsterdam
Ming Tang Chen
Academia Sinica
Yongjun Chen
Chinese Academy of Sciences
I. Cho
University of Science and Technology (UST)
Korea Astronomy and Space Science Institute
Pierre Christian
Harvard-Smithsonian Center for Astrophysics
University of Arizona
John Conway
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
James M. Cordes
Cornell University
G. Crew
Massachusetts Institute of Technology (MIT)
Yuzhu Cui
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
Jordy Davelaar
Radboud Universiteit
Mariafelicia De Laurentis
Johann Wolfgang Goethe Universität Frankfurt am Main
Universita degli Studi di Napoli Federico II
R. P. Deane
Rhodes University
Universiteit van Pretoria
Jessica Dempsey
East Asian Observatory
Gregory Desvignes
Max-Planck-Gesellschaft
Jason Dexter
Max-Planck-Gesellschaft
S. Doeleman
Harvard University
Harvard-Smithsonian Center for Astrophysics
Ralph P. Eatough
Max-Planck-Gesellschaft
H.D. Falcke
Radboud Universiteit
V. Fish
Massachusetts Institute of Technology (MIT)
Ed Fomalont
National Radio Astronomy Observatory
R. Fraga-Encinas
Radboud Universiteit
P. Friberg
East Asian Observatory
Christian M. Fromm
Johann Wolfgang Goethe Universität Frankfurt am Main
J. L. Gomez
Consejo Superior de Investigaciones Científicas (CSIC)
Peter Galison
Harvard University
Charles F. Gammie
University of Illinois
Roberto Garcia
Institut de Radioastronomie Millimétrique (IRAM)
Olivier Gentaz
Institut de Radioastronomie Millimétrique (IRAM)
Boris Georgiev
University of Waterloo
C. Goddi
Universiteit Leiden
Radboud Universiteit
R. Gold
Johann Wolfgang Goethe Universität Frankfurt am Main
Minfeng Gu
Chinese Academy of Sciences
M. Gurwell
Harvard-Smithsonian Center for Astrophysics
K. Hada
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
Michael H. Hecht
Massachusetts Institute of Technology (MIT)
R. Hesper
Rijksuniversiteit Groningen
Luis C. Ho
Beijing University of Technology
P. T. P. Ho
National Taiwan University
Mareki Honma
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
Chih Wei L. Huang
National Taiwan University
Lei Huang
Chinese Academy of Sciences
D. Hughes
Instituto Nacional de Astrofísica, Óptica y Electrońica
Shiro Ikeda
The Institute of Statistical Mathematics
The Graduate University for Advanced Studies (SOKENDAI)
University of Tokyo
National Astronomical Observatory of Japan
Makoto Inoue
National Taiwan University
S. Issaoun
Radboud Universiteit
David J. James
Harvard-Smithsonian Center for Astrophysics
Harvard University
Buell T. Jannuzi
University of Arizona
M. Janßen
Radboud Universiteit
Britton Jeter
University of Waterloo
Wu Jiang
Chinese Academy of Sciences
Michael D. Johnson
Harvard University
Harvard-Smithsonian Center for Astrophysics
S.G. Jorstad
Boston University
Saint Petersburg State University - Spsu
Taehyun Jung
University of Science and Technology (UST)
Korea Astronomy and Space Science Institute
Mansour Karami
Perimeter Institute for Theoretical Physics
University of Waterloo
R. Karuppusamy
Max-Planck-Gesellschaft
Tomohisa Kawashima
National Astronomical Observatory of Japan
G. Keating
Harvard-Smithsonian Center for Astrophysics
M. M. Kettenis
Joint Institute for VLBI in Europe (JIVE)
Jae Young Kim
Max-Planck-Gesellschaft
Junhan Kim
University of Arizona
Jongsoo Kim
Korea Astronomy and Space Science Institute
M. Kino
Kogakuin University of Technology and Engineering
National Astronomical Observatory of Japan
Jun Yi Koay
National Taiwan University
Patrick M. Koch
National Taiwan University
Shoko Koyama
National Taiwan University
M. Kramer
Max-Planck-Gesellschaft
C. Kramer
Institut de Radioastronomie Millimétrique (IRAM)
T.P. Krichbaum
Max-Planck-Gesellschaft
Cheng Yu Kuo
National Sun Yat-Sen University
Tod R. Lauer
National Optical Astronomy Observatory
Sang Sung Lee
Korea Astronomy and Space Science Institute
Yan Rong Li
Chinese Academy of Sciences
Zhiyuan Li
Nanjing University
Publicerad i
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 875 Nummer/häfte 1 art. nr L2Kategorisering
Ämneskategorier (SSIF 2011)
Rymd- och flygteknik
Astronomi, astrofysik och kosmologi
Identifikatorer
DOI
10.3847/2041-8213/ab0c96