Geometric Parallax

Geometric Parallax is a measurement method in astrometry that determines the distance to a celestial object by observing its apparent shift in position relative to background stars from two distinct vantage points, using the principles of triangulation.

65

Publications

4.5K

Citations

181

Authors

103

Institutions

Publications per year

2017–2026

16

Authors

181

  1. AT
    Adam T. Deller

    Swinburne University of Technology, Australia

    3 publications · 92 citations

    3

    h-index

  2. SC
    Shami Chatterjee

    Cornell University, United States

    2 publications · 49 citations

    2

    h-index

  3. WD
    Weiqiang Ding

    Harbin Institute of Technology, China

    2 publications · 23 citations

    2

    h-index

  4. BR
    Brian Rogers

    University of Oxford, United Kingdom

    2 publications · 61 citations

    2

    h-index

  5. JG
    Jie Gong

    Goddard Space Flight Center, United States

    2 publications · 30 citations

    2

    h-index

1–5 of 181

Venues

  1. The Astrophysical Journal

    ApJ · 7 publications · 406 citations

    7

    h-index

  2. 4

    h-index

  3. The Astronomical Journal

    AJ · 4 publications · 2K citations

    4

    h-index

  4. Journal for the History of Astronomy

    JHA · 2 publications · 44 citations

    2

    h-index

  5. Optics Express

    2 publications · 78 citations

    2

    h-index

1–5