Testing Planet Formation Models with Gaia as Astrometry
arXiv:0711.4903 · doi:10.1017/S1743921308019200
Abstract
In this paper, we first summarize the results of a large-scale double-blind tests campaign carried out for the realistic estimation of the Gaia potential in detecting and measuring planetary systems. Then, we put the identified capabilities in context by highlighting the unique contribution that the Gaia exoplanet discoveries will be able to bring to the science of extrasolar planets during the next decade.
4 pages, 1 figure. To appear in the proceedings of "IAU Symposium 248 - A Giant Step: from Milli- to Micro-arcsecond Astrometry", held in Shanghai, China, 15-19 Oct. 2007
References in corpus (5)
- GAIA: Composition, Formation and Evolution of the Galaxy
- Maximum likelihood method for estimating the mass and period distributions of extra-solar planets
- The Mass of the Candidate Exoplanet Companion to HD 33636 from Hubble Space Telescope Astrometry and High-Precision Radial Velocities
- Astrometric Methods and Instrumentation to Identify and Characterize Extrasolar Planets: A Review
- Space-borne global astrometric surveys: the hunt for extra-solar planets