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

Citations

55

Authors

40

Institutions

Publications per year

2017–2026

3

Authors

55

  1. SL
    Stephen L. Trokel

    Columbia University, United States

    1 publications · 78 citations

    1

    h-index

  2. JL
    J.-B. Le Bouquin

    Centre National de la Recherche Scientifique, France

    1 publications · 14 citations

    1

    h-index

  3. RA
    Robert A. Jacobson

    Iowa State University, United States

    1 publications · 30 citations

    1

    h-index

  4. RR
    Robin R. Richards

    St. Michael's Hospital, Canada

    1 publications · 71 citations

    1

    h-index

  5. QW
    Qian Wang

    University of Massachusetts Lowell, United States

    1 publications · 11 citations

    1

    h-index

1–5 of 55

Venues

  1. Medical Physics

    2 publications · 23 citations

    2

    h-index

  2. arXiv (Cornell University)

    Repository · 1 publications · 25 citations

    1

    h-index

  3. Journal of Oral and Maxillofacial Surgery

    1 publications · 86 citations

    1

    h-index

  4. The Journal of the Astronautical Sciences

    1 publications · 30 citations

    1

    h-index

  5. The Astrophysical Journal Supplement Series

    1 publications · 142 citations

    1

    h-index

1–5