orbitize! v3: Orbit fitting for the High-contrast Imaging Community

orbitize! is a package for Bayesian modeling of the orbital parameters of resolved binary objects from time series measurements. It was developed with the needs of the high-contrast imaging community in mind, and has since also become widely used in the binary star community. A generic orbitize! use...

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Vydáno v:Journal of open source software Ročník 9; číslo 101; s. 6756
Hlavní autoři: Blunt, Sarah, Wang, Jason J, Hirsch, Lea, Tejada, Roberto, Nagpal, Vighnesh, Surti, Tirth Dharmesh, Covarrubias, Sofia, McKenna, Thea, Chávez, Rodrigo Ferrer, Llop-Sayson, Jorge, Arora, Mireya, Chavez, Amanda, Cody, Devin, Choudhary, Saanika, Smith, Adam J R W, Balmer, William, Stolker, Tomas, Gallamore, Hannah, Ó, Clarissa R Do, Nielsen, Eric L, Rosa, Robert J De
Médium: Journal Article
Jazyk:angličtina
Vydáno: 2230 Support Open Journals 21.09.2024
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ISSN:2475-9066, 2475-9066
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Popis
Shrnutí:orbitize! is a package for Bayesian modeling of the orbital parameters of resolved binary objects from time series measurements. It was developed with the needs of the high-contrast imaging community in mind, and has since also become widely used in the binary star community. A generic orbitize! use case involves translating relative astrometric time series, optionally combined with radial velocity or astrometric time series, into a set of derived orbital posteriors. This paper is published alongside the release of orbitize! version 3.0, which has seen significant enhancements in functionality and accessibility since the release of version 1.0 (Blunt et al., 2020).
Bibliografie:2230 Support
2230
ISSN:2475-9066
2475-9066
DOI:10.21105/joss.06756