Stellar Parallax

Stellar Parallax is the apparent angular displacement of a nearby star against the background of distant stars, observed from two different positions in Earth's orbit around the Sun, used as a foundational method in astrometry for directly measuring astronomical distances.

825

Publications

64.9K

Citations

3.7K

Authors

708

Institutions

Publications per year

2017–2026

228

Authors

3.7K

  1. MJ
    M. J. Reid

    Center for Astrophysics Harvard & Smithsonian, United States

    27 publications · 3.5K citations

    25

    h-index

  2. KM
    K. M. Menten

    Max Planck Institute for Radio Astronomy, Germany

    24 publications · 3.4K citations

    23

    h-index

  3. LE
    L. Eyer

    University of Geneva, Switzerland

    23 publications · 2.6K citations

    22

    h-index

  4. AB
    A. Brunthaler

    Max Planck Institute for Radio Astronomy, Germany

    22 publications · 3.2K citations

    21

    h-index

  5. GM
    G. M. Seabroke

    University College London, United Kingdom

    21 publications · 2.9K citations

    20

    h-index

1–5 of 3.7K

Venues

  1. The Astrophysical Journal

    ApJ · 181 publications · 15.3K citations

    72

    h-index

  2. Astronomy and Astrophysics

    145 publications · 15.7K citations

    62

    h-index

  3. The Astronomical Journal

    AJ · 123 publications · 13.3K citations

    51

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    108 publications · 5.4K citations

    41

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 29 publications · 1.1K citations

    16

    h-index

1–5