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
153
The International Celestial Reference Frame as Realized by Very Long Baseline Interferometry
Chao Ma, E. F. Arias, T. M. Eubanks et al. · The Astronomical Journal · 1998 · 775 citations · Full text
Natural Sciences, Astronomy, Physics +14
Coordinate systems for solar image data
W. T. Thompson · Astronomy and Astrophysics · 2006 · 380 citations · Full text
1–5 of 153
484
10
h-index
9
h-index
9
h-index
8
h-index
8
h-index
1–5 of 484
197
United States Naval Observatory
Flagstaff, United States
26 h-index
45 publications
6.6K citations

Centre National de la Recherche Scientifique
Paris, France
21 h-index
90 publications
6.7K citations

Observatoire de Paris
Paris, France
17 h-index
52 publications
7.4K citations
Institute of Applied Astronomy
Saint Petersburg, Russia
15 h-index
17 publications
2K citations
Jet Propulsion Laboratory
Pasadena, United States
15 h-index
31 publications
3.5K citations
Systèmes de Référence Temps-Espace
Paris, France
15 h-index
67 publications
3.1K citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
24 publications
3.9K citations

Sorbonne Université
Paris, France
10 h-index
36 publications
1.6K citations
1–8 of 197
35 publications · 1.7K citations
20
h-index
AJ · 22 publications · 2.4K citations
18
h-index
10 publications · 1.1K citations
10
h-index
9 publications · 1.5K citations
9
h-index
6 publications · 137 citations
6
h-index
1–5