Absolute Proper Motion
Absolute Proper Motion is a celestial kinematic measurement that quantifies the apparent angular shift of a star or astronomical object on the sky relative to a fixed inertial reference frame, distinguished from relative proper motion by its correction for solar system barycentric motion and its anchoring to extragalactic or distant reference sources to establish an absolute standard of rest.
222
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12K
Citations
740
Authors
340
Institutions
Publications per year
2017–2026
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Precise proper-motion measurement of solar granulation
L. J. November, George W. Simon · The Astrophysical Journal · 1988 · 461 citations
Natural Sciences, Astronomy, Physics +15
OGLE‐2003‐BLG‐262: Finite‐Source Effects from a Point‐Mass Lens
The Astrophysical Journal · 2004 · 412 citations · Full text
Natural Sciences, Astronomy, Physics +12
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Space Telescope Science Institute
Baltimore, United States
25 h-index
76 publications
4.5K citations
Yale University
New Haven, United States
22 h-index
83 publications
5.5K citations
University of Virginia
Charlottesville, United States
17 h-index
39 publications
2K citations
Osservatorio Astronomico di Padova
Padua, Italy
14 h-index
40 publications
3.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
22 publications
2K citations
Université Bourgogne Franche-Comté
Besançon, France
14 h-index
37 publications
1.6K citations

Romanian Academy
Bucharest, Romania
13 h-index
13 publications
616 citations

Johns Hopkins University
Baltimore, United States
11 h-index
17 publications
1.2K citations
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AJ · 54 publications · 3.3K citations
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ApJ · 51 publications · 3.6K citations
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35 publications · 1.4K citations
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21 publications · 1.1K citations
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8 publications · 311 citations
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