Extragalactic Proper Motion

Extragalactic Proper Motion is a measurement methodology in astrometry that quantifies the apparent angular displacement over time of extragalactic celestial objects across the plane of the sky, distinguishing it from galactic proper motion by focusing on sources beyond the Milky Way and requiring corrections for cosmological effects and reference frame stability.

128

Publications

9.7K

Citations

1.2K

Authors

330

Institutions

Publications per year

2017–2026

37

Authors

1.2K

  1. LL
    L. Lindegren

    Lund University, Sweden

    8 publications · 1.1K citations

    8

    h-index

  2. DW
    D. W. Evans

    University of Cambridge, United Kingdom

    7 publications · 1.2K citations

    7

    h-index

  3. CF
    C. Fabricius

    Universitat de Barcelona, Spain

    7 publications · 1.2K citations

    7

    h-index

  4. AG
    A. G. A. Brown

    Leiden University, Netherlands

    7 publications · 1.2K citations

    7

    h-index

  5. JP
    J. Portell

    Universitat de Barcelona, Spain

    7 publications · 1.2K citations

    7

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 23 publications · 2.8K citations

    20

    h-index

  2. The Astronomical Journal

    AJ · 22 publications · 1.5K citations

    19

    h-index

  3. Astronomy and Astrophysics

    18 publications · 1.9K citations

    17

    h-index

  4. Nature

    11 publications · 595 citations

    11

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    12 publications · 1.1K citations

    10

    h-index

1–5