Three-dimensional Orbit Reconstruction
Three-Dimensional Orbit Reconstruction is a computational method in astrophysics that, within the study of binary star systems, uniquely determines the full spatial trajectory and orientation of an orbit by integrating observational data with dynamical modeling to recover the three-dimensional geometry from projected two-dimensional measurements.
17
Publications
625
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55
Authors
40
Institutions
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2017–2026
3
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17
Axisymmetric Three‐Integral Models for Galaxies
N. Cretton, P. T. de Zeeuw, Roeland P. van der Marel et al. · The Astrophysical Journal Supplement Series · 1999 · 142 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Stanford University
Stanford, United States
2 h-index
6 publications
68 citations

Université Grenoble Alpes
Saint-Martin-d'Hères, France
1 h-index
5 publications
70 citations
Leiden University
Leiden, The Netherlands
1 h-index
2 publications
284 citations
University of Arizona
Tucson, United States
1 h-index
1 publications
142 citations
Stanford Medicine
Stanford, United States
1 h-index
1 publications
12 citations

Centre National de la Recherche Scientifique
Paris, France
1 h-index
5 publications
70 citations

University College Hospital
London, United Kingdom
1 h-index
1 publications
71 citations
Université de Strasbourg
Strasbourg, France
1 h-index
3 publications
54 citations
1–8 of 40
2 publications · 23 citations
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Repository · 1 publications · 25 citations
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1 publications · 86 citations
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1 publications · 30 citations
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1 publications · 142 citations
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