2011/07/01 by L. Eyer, P. Dubath, N. Mowlavi +13
Physics and Astronomy · #Astronomy and Astrophysical Research #Binary number #Exoplanet #History and Developments in Astronomy #Planet #Radial velocity #Range (aeronautics) #Scale (ratio) #Stellar, planetary, and galactic studies #astro-ph.IM #astro-ph.SR
paper · pdf · doi:10.1017/s1743921311026822
8 pages, 2 figures, Proceedings of the IAU Symposium No. 282: From Interacting Binaries to Exoplanets: Essential Modeling Tools. Tatranska Lomnica, Slovakia
openalex publication_date 2011/07/01 · arxiv created 2012/01/24 · arxiv updated 2015/06/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Abstract Two upcoming large scale surveys, the ESA Gaia and LSST projects, will bring a new era in astronomy. The number of binary systems that will be observed and detected by these projects is enormous, estimations range from millions for Gaia to several tens of millions for LSST. We review some tools that should be developed and also what can be gained from these missions on the subject of binaries and exoplanets from the astrometry, photometry, radial velocity and their alert systems.