Very Long Baseline Interferometry
Very Long Baseline Interferometry is a specialized form of astronomical interferometry that achieves extremely high angular resolution by synchronously recording electromagnetic wavefronts from widely separated radio telescopes and later correlating the data using precise timing references, thereby synthesizing an aperture comparable to the baseline distance between the telescopes.
1K
Publications
72.8K
Citations
3.9K
Authors
947
Institutions
Publications per year
2017–2026
253
Variants
Vlbi
Parents
1K
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
Kazunori Akiyama, A. Alberdi, W. Alef et al. · The Astrophysical Journal Letters · 2019 · 4.2K citations · Full text
Natural Sciences, Astronomy, Physics +12
1–5 of 1K
3.9K
25
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25
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Center for Astrophysics Harvard & Smithsonian, United States
30 publications · 7K citations
24
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24
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23
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1–5 of 3.9K
947
Max Planck Institute for Radio Astronomy
Bonn, Germany
53 h-index
761 publications
217.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
46 h-index
482 publications
190.7K citations
National Radio Astronomy Observatory
Charlottesville, United States
45 h-index
199 publications
55.8K citations

Centre National de la Recherche Scientifique
Paris, France
39 h-index
333 publications
51.9K citations
Massachusetts Institute of Technology
Cambridge, United States
36 h-index
295 publications
139K citations
California Institute of Technology
Pasadena, United States
35 h-index
164 publications
27.2K citations
Goddard Space Flight Center
Greenbelt, United States
34 h-index
118 publications
10K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
34 h-index
401 publications
107.8K citations
1–8 of 947
ApJ · 149 publications · 9.3K citations
48
h-index
131 publications · 5.4K citations
42
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JGR · 78 publications · 9.8K citations
42
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114 publications · 5.8K citations
40
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AJ · 59 publications · 3.9K citations
33
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