Celestial Reference Systems

Celestial Reference Systems is a coordinate framework used in geodetic astronomy to define the precise positions and motions of celestial objects relative to the Earth’s rotation by establishing a fixed inertial reference aligned with distant quasars and realized through extragalactic radio sources.

153

Publications

10.2K

Citations

484

Authors

197

Institutions

Publications per year

2017–2026

13

Variants

Celestial Reference System

Authors

484

  1. PK
    P. K. Seidelmann

    United States Naval Observatory, United States

    10 publications · 1.4K citations

    10

    h-index

  2. NC
    N. Capitaine

    Centre National de la Recherche Scientifique, France

    9 publications · 791 citations

    9

    h-index

  3. PC
    P. Charlot

    Centre National de la Recherche Scientifique, France

    9 publications · 1.4K citations

    9

    h-index

  4. CM
    Chao Ma

    Goddard Space Flight Center, United States

    8 publications · 1.9K citations

    8

    h-index

  5. AH
    A. H. Andrei

    National Observatory, Brazil

    8 publications · 195 citations

    8

    h-index

1–5 of 484

Venues

  1. Astronomy and Astrophysics

    35 publications · 1.7K citations

    20

    h-index

  2. The Astronomical Journal

    AJ · 22 publications · 2.4K citations

    18

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    10 publications · 1.1K citations

    10

    h-index

  4. 9

    h-index

  5. Journal of Geodesy

    6 publications · 137 citations

    6

    h-index

1–5