Milliarcsecond Astrometry

Milliarcsecond Astrometry is a high-precision observational technique in positional astronomy that achieves angular measurements on the order of milliarcseconds to determine the exact positions, distances, and motions of celestial objects with exceptional accuracy.

46

Publications

2.2K

Citations

280

Authors

184

Institutions

Publications per year

2017–2026

13

Authors

280

  1. KJ
    K. J. Johnston

    United States Naval Observatory, United States

    4 publications · 109 citations

    4

    h-index

  2. SP
    S. P. Ellingsen

    University of Tasmania, Australia

    4 publications · 77 citations

    4

    h-index

  3. ES
    E. Slezak

    Observatoire de la Côte d’Azur, France

    3 publications · 49 citations

    3

    h-index

  4. RT
    R. Teixeira

    Centre National de la Recherche Scientifique, France

    3 publications · 49 citations

    3

    h-index

  5. FM
    F. Mignard

    Observatoire de la Côte d’Azur, France

    3 publications · 49 citations

    3

    h-index

1–5 of 280

Venues

  1. The Astronomical Journal

    AJ · 12 publications · 684 citations

    11

    h-index

  2. Astronomy and Astrophysics

    5 publications · 130 citations

    5

    h-index

  3. The Astrophysical Journal

    ApJ · 4 publications · 166 citations

    4

    h-index

  4. arXiv (Cornell University)

    Repository · 2 publications · 31 citations

    2

    h-index

  5. 2

    h-index

1–5