Proper Motion
Proper Motion is the apparent angular displacement of a celestial object on the celestial sphere, distinguished from other types of observed motion by representing the gradual change in position relative to distant background stars over time due to the object's true motion through space.
3.5K
Publications
251.9K
Citations
8.7K
Authors
1.4K
Institutions
Publications per year
2017–2026
842
3.5K
The Astronomical Journal · 2003 · 2.1K citations · Full text
Natural Sciences, Astronomy, Physics +16
A statistical study of 233 pulsar proper motions
Monthly Notices of the Royal Astronomical Society · 2005 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 3.5K
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Center for Astrophysics Harvard & Smithsonian, United States
40 publications · 6K citations
30
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1–5 of 8.7K
1.4K
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
86 h-index
542 publications
180K citations

Space Telescope Science Institute
Baltimore, United States
75 h-index
532 publications
43.6K citations

Centre National de la Recherche Scientifique
Paris, France
72 h-index
1.3K publications
175.8K citations
University of Cambridge
Cambridge, United Kingdom
68 h-index
470 publications
68K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
63 h-index
388 publications
39.6K citations
California Institute of Technology
Pasadena, United States
61 h-index
321 publications
47.2K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
60 h-index
421 publications
207.5K citations
Université Bourgogne Franche-Comté
Besançon, France
53 h-index
311 publications
31.7K citations
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ApJ · 835 publications · 66.5K citations
131
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599 publications · 38.8K citations
96
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AJ · 486 publications · 39K citations
96
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461 publications · 32.2K citations
90
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69 publications · 6.1K citations
41
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