Proper Motion Determination
Proper Motion Determination is a methodological framework in astrometry that quantifies the apparent angular motion of celestial objects across the sky over time by systematically measuring and analyzing position changes relative to distant background reference sources, thereby distinguishing intrinsic stellar or planetary kinematics from observational artifacts.
609
Publications
37.6K
Citations
1.9K
Authors
601
Institutions
Publications per year
2017–2026
127
609
Gaia Data Release 2. The astrometric solution
L. Lindegren, J. Hernández, A. Bombrun et al. · arXiv (Cornell University) · 2018 · 932 citations · Full text
Natural Sciences, Astronomy, Physics +17
Observations of stellar proper motions near the Galactic Centre
A. Eckart, R. Genzel · Nature · 1996 · 439 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 609
1.9K
12
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10
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10
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Space Telescope Science Institute, United States
9 publications · 944 citations
9
h-index
9
h-index
1–5 of 1.9K
601

Space Telescope Science Institute
Baltimore, United States
34 h-index
140 publications
11.6K citations

Centre National de la Recherche Scientifique
Paris, France
33 h-index
136 publications
9.3K citations
California Institute of Technology
Pasadena, United States
31 h-index
105 publications
9.4K citations
Université Bourgogne Franche-Comté
Besançon, France
27 h-index
85 publications
5K citations
University of Arizona
Tucson, United States
25 h-index
36 publications
3.1K citations
European Southern Observatory
Santiago, Chile
25 h-index
41 publications
2.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
25 h-index
69 publications
5K citations
Jet Propulsion Laboratory
Pasadena, United States
24 h-index
54 publications
4.7K citations
1–8 of 601
ApJ · 133 publications · 10.1K citations
55
h-index
AJ · 125 publications · 8.4K citations
48
h-index
105 publications · 5.8K citations
45
h-index
97 publications · 5.3K citations
39
h-index
12 publications · 267 citations
11
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1–5