Absolute Proper Motion

Absolute Proper Motion is a celestial kinematic measurement that quantifies the apparent angular shift of a star or astronomical object on the sky relative to a fixed inertial reference frame, distinguished from relative proper motion by its correction for solar system barycentric motion and its anchoring to extragalactic or distant reference sources to establish an absolute standard of rest.

222

Publications

12K

Citations

740

Authors

340

Institutions

Publications per year

2017–2026

41

Authors

740

  1. TM
    Terrence M. Girard

    Yale University, United States

    23 publications · 1.6K citations

    18

    h-index

  2. WF
    W. F. van Altena

    Yale University, United States

    17 publications · 1.3K citations

    16

    h-index

  3. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    14 publications · 901 citations

    13

    h-index

  4. SR
    Steven R. Majewski

    University of Virginia, United States

    13 publications · 804 citations

    13

    h-index

  5. DI
    Dana I. Dinescu

    Yale University, United States

    12 publications · 1.1K citations

    12

    h-index

1–5 of 740

Venues

  1. The Astronomical Journal

    AJ · 54 publications · 3.3K citations

    34

    h-index

  2. The Astrophysical Journal

    ApJ · 51 publications · 3.6K citations

    31

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    35 publications · 1.4K citations

    20

    h-index

  4. Astronomy and Astrophysics

    21 publications · 1.1K citations

    18

    h-index

  5. Astronomy and Astrophysics Supplement Series

    8 publications · 311 citations

    8

    h-index

1–5