The Exoplanet Simple Orbit Fitting Toolbox (ExoSOFT): An Open-source Tool for Efficient Fitting of Astrometric and Radial Velocity Data

被引:17
|
作者
Mede, Kyle [1 ]
Brandt, Timothy D. [2 ]
机构
[1] Univ Tokyo, Tokyo, Japan
[2] Inst Adv Study, Olden Lane, Princeton, NJ 08540 USA
来源
ASTRONOMICAL JOURNAL | 2017年 / 153卷 / 03期
关键词
astrometry; brown dwarfs; methods: statistical; planetary systems; techniques: high angular resolution; techniques: radial velocities; GIANT PLANET FORMATION; SOLAR-TYPE STARS; HR; 8799; PLANETS; ECCENTRICITY DISTRIBUTION; EXTRASOLAR PLANETS; BROWN DWARFS; MASS FUNCTION; MONTE-CARLO; 1ST LIGHT; COMPANION;
D O I
10.3847/1538-3881/aa5e4a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the Exoplanet Simple Orbit Fitting Toolbox (ExoSOFT), a new, open-source suite to fit the orbital elements of planetary or stellar-mass companions to any combination of radial velocity and astrometric data. To explore the parameter space of Keplerian models, ExoSOFT may be operated with its own multistage sampling approach or interfaced with third-party tools such as emcee. In addition, ExoSOFT is packaged with a collection of post-processing tools to analyze and summarize the results. Although only a few systems have been observed with both radial velocity and direct imaging techniques, this number will increase, thanks to upcoming spacecraft and ground-based surveys. Providing both forms of data enables simultaneous fitting that can help break degeneracies in the orbital elements that arise when only one data type is available. The dynamical mass estimates this approach can produce are important when investigating the formation mechanisms and subsequent evolution of substellar companions. ExoSOFT was verified through fitting to artificial data and was implemented using the Python and Cython programming languages; it is available for public download at https://github.com/kylemede/ExoSOFT under. GNU General Public License v3.
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页数:9
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