Extragalactic Proper Motion
Extragalactic Proper Motion is a measurement methodology in astrometry that quantifies the apparent angular displacement over time of extragalactic celestial objects across the plane of the sky, distinguishing it from galactic proper motion by focusing on sources beyond the Milky Way and requiring corrections for cosmological effects and reference frame stability.
128
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9.7K
Citations
1.2K
Authors
330
Institutions
Publications per year
2017–2026
37
Parents
128
The Proper Motion of Sagittarius A*. II. The Mass of Sagittarius A*
M. J. Reid, A. Brunthaler · The Astrophysical Journal · 2004 · 799 citations · Full text
Natural Sciences, Astronomy, Physics +15
<i>Gaia</i> Early Data Release 3
R. L. Smart, L. M. Sarro, J. Rybizki et al. · Astronomy and Astrophysics · 2020 · 330 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
40 publications
4.2K citations

Centre National de la Recherche Scientifique
Paris, France
15 h-index
320 publications
56.5K citations

Space Telescope Science Institute
Baltimore, United States
12 h-index
31 publications
3.4K citations
California Institute of Technology
Pasadena, United States
12 h-index
16 publications
1.8K citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
11 h-index
27 publications
4K citations

University of Edinburgh
Edinburgh, United Kingdom
10 h-index
37 publications
6.2K citations
University of Cambridge
Cambridge, United Kingdom
10 h-index
126 publications
21.3K citations
Jet Propulsion Laboratory
Pasadena, United States
10 h-index
12 publications
1.4K citations
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ApJ · 23 publications · 2.8K citations
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AJ · 22 publications · 1.5K citations
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18 publications · 1.9K citations
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11 publications · 595 citations
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12 publications · 1.1K citations
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