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arXiv:0711.4903 (astro-ph)
[Submitted on 30 Nov 2007]

Title:Testing Planet Formation Models with Gaia $μ$as Astrometry

Authors:A. Sozzetti (1,2), S. Casertano (3), M.G. Lattanzi (2), A. Spagna (1), R. Morbidelli (2), R. Pannunzio (2), D. Pourbaix (4), D. Queloz (5) ((1) CfA, (2) OATo, (3) STScI, (4)ULB, (5)Geneva)
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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.
Comments: 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
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0711.4903 [astro-ph]
  (or arXiv:0711.4903v1 [astro-ph] for this version)
  https://doi.org/10.48550/arXiv.0711.4903
Related DOI: https://doi.org/10.1017/S1743921308019200

Submission history

From: Alessandro Sozzetti [view email]
[v1] Fri, 30 Nov 2007 11:10:12 UTC (42 KB)
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