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

Authors

3.9K

  1. AE
    A. E. E. Rogers

    Massachusetts Institute of Technology, United States

    33 publications · 8.5K citations

    25

    h-index

  2. JA
    J. A. Zensus

    Max Planck Institute for Radio Astronomy, Germany

    41 publications · 7.4K citations

    25

    h-index

  3. SS
    Sheperd S. Doeleman

    Center for Astrophysics Harvard & Smithsonian, United States

    30 publications · 7K citations

    24

    h-index

  4. TP
    T. P. Krichbaum

    Max Planck Institute for Radio Astronomy, Germany

    39 publications · 6.7K citations

    24

    h-index

  5. AP
    A. P. Lobanov

    Max Planck Institute for Radio Astronomy, Germany

    31 publications · 6.5K citations

    23

    h-index

1–5 of 3.9K

Venues

  1. The Astrophysical Journal

    ApJ · 149 publications · 9.3K citations

    48

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    131 publications · 5.4K citations

    42

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 78 publications · 9.8K citations

    42

    h-index

  4. Astronomy and Astrophysics

    114 publications · 5.8K citations

    40

    h-index

  5. The Astronomical Journal

    AJ · 59 publications · 3.9K citations

    33

    h-index

1–5