Keplerian Orbit Fitting is a computational method in astrophysics that belongs to the class of orbital parameter estimation techniques, specifically designed to determine the orbital elements of a binary star system by modeling observational data according to Kepler's laws of planetary motion.
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2017–2026
13
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Keplerian Orbit Determination
Parents
Publications
75
The generalised Lomb-Scargle periodogram
M. Zechmeister, M. Kürster · Astronomy and Astrophysics · 2009 · 1.7K citations · Full text
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University of California, Berkeley
Berkeley, United States
12 h-index
36 publications
7.1K citations
California Institute of Technology
Pasadena, United States
10 h-index
19 publications
2.7K citations
Centre National de la Recherche Scientifique
Paris, France
8 h-index
16 publications
484 citations
University of California, Santa Cruz
Santa Cruz, United States
8 h-index
16 publications
4.9K citations
San Francisco State University
San Francisco, United States
8 h-index
12 publications
2.5K citations
Carnegie Institution for Science
Washington, United States
8 h-index
8 publications
679 citations
Carnegie Observatories
Pasadena, United States
7 h-index
7 publications
669 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
18 publications
655 citations
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- The Astrophysical Journal
ApJ · 21 publications · 1.9K citations
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- Monthly Notices of the Royal Astronomical Society
10 publications · 592 citations
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- Astronomy and Astrophysics
7 publications · 1.9K citations
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- The Astronomical Journal
AJ · 6 publications · 318 citations
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- CERN Document Server (European Organization for Nuclear Research)
Repository · 3 publications · 241 citations
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