Proper Motion Estimation

Proper Motion Estimation is a computational method in astrometry that determines the intrinsic angular displacement of a celestial object on the sky over time by disentangling its motion from observational artifacts and reference frame effects.

244

Publications

14.1K

Citations

674

Authors

342

Institutions

Publications per year

2017–2026

48

Authors

674

  1. TM
    Terrence M. Girard

    Yale University, United States

    9 publications · 500 citations

    9

    h-index

  2. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    9 publications · 587 citations

    9

    h-index

  3. LL
    L. Lindegren

    Lund University, Sweden

    7 publications · 518 citations

    7

    h-index

  4. RP
    Roeland P. van der Marel

    Space Telescope Science Institute, United States

    5 publications · 873 citations

    5

    h-index

  5. VD
    V. D. Ivanov

    European Southern Observatory, Chile

    5 publications · 147 citations

    5

    h-index

1–5 of 674

Venues

  1. Astronomy and Astrophysics

    55 publications · 3K citations

    30

    h-index

  2. The Astrophysical Journal

    ApJ · 48 publications · 4.4K citations

    29

    h-index

  3. The Astronomical Journal

    AJ · 43 publications · 2.6K citations

    25

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    31 publications · 1.1K citations

    19

    h-index

  5. Astronomische Nachrichten

    6 publications · 104 citations

    6

    h-index

1–5