Topocentric Coordinates
Topocentric Coordinates is a coordinate system in solar system astrometry that specifies the position of a celestial object relative to an observer's location on the surface of the Earth, differing from geocentric or heliocentric systems by accounting for the observer's local topography and parallax effects.
18
Publications
711
Citations
49
Authors
29
Institutions
Publications per year
2017–2026
4
18
Topocentric orbit determination: Algorithms for the next generation surveys
Andrea Milani, Giovanni F. Gronchi, Davide Farnocchia et al. · Icarus · 2008 · 35 citations · Full text
Natural Sciences, Astronomy, Geodesy +13
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49
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29
Goddard Space Flight Center
Greenbelt, United States
4 h-index
5 publications
149 citations

University of Pisa
Pisa, Italy
2 h-index
5 publications
133 citations

Centre National de la Recherche Scientifique
Paris, France
2 h-index
2 publications
62 citations
New York University
New York, United States
1 h-index
3 publications
588 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
1 h-index
1 publications
29 citations

University of Naples Federico II
Naples, Italy
1 h-index
1 publications
15 citations

University of Hawaii System
Honolulu, United States
1 h-index
2 publications
70 citations
George Mason University
Fairfax, United States
1 h-index
1 publications
33 citations
1–8 of 29
AJ · 2 publications · 45 citations
2
h-index
Repository · 2 publications · 70 citations
2
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2 publications · 34 citations
2
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ApJ · 1 publications · 33 citations
1
h-index
1 publications · 15 citations
1
h-index
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