Proper Motion Determination

Proper Motion Determination is a methodological framework in astrometry that quantifies the apparent angular motion of celestial objects across the sky over time by systematically measuring and analyzing position changes relative to distant background reference sources, thereby distinguishing intrinsic stellar or planetary kinematics from observational artifacts.

609

Publications

37.6K

Citations

1.9K

Authors

601

Institutions

Publications per year

2017–2026

127

Authors

1.9K

  1. TM
    Terrence M. Girard

    Yale University, United States

    12 publications · 553 citations

    12

    h-index

  2. MM
    M. Mugrauer

    Friedrich Schiller University Jena, Germany

    10 publications · 405 citations

    10

    h-index

  3. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    10 publications · 623 citations

    10

    h-index

  4. RP
    Roeland P. van der Marel

    Space Telescope Science Institute, United States

    9 publications · 944 citations

    9

    h-index

  5. DM
    D. Minniti

    Pontificia Universidad Católica de Chile, Chile

    9 publications · 475 citations

    9

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 133 publications · 10.1K citations

    55

    h-index

  2. The Astronomical Journal

    AJ · 125 publications · 8.4K citations

    48

    h-index

  3. Astronomy and Astrophysics

    105 publications · 5.8K citations

    45

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    97 publications · 5.3K citations

    39

    h-index

  5. Astronomische Nachrichten

    12 publications · 267 citations

    11

    h-index

1–5