2015/01/31 by J. Lillo-Box, D. Barrado, L. Mancini +5
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Eccentricity (behavior) #Eclipse #Exoplanet #Kepler #Light curve #Observatory #Orbit (dynamics) #Physics #Planet #Planetary system #Radial velocity #Spectral line #Spectrograph #Stars #Stellar, planetary, and galactic studies #astro-ph.EP
paper · pdf · doi:10.1051/0004-6361/201425272
published as A&A 576, A88 (2015) · Accepted for publication in A&A. 18 pages, 9 figures, 17 tables. This version fixes an error affecting the values of tables A.1-A.13. The text remains unaltered
openalex publication_date 2015/02/10 · arxiv created 2015/02/17 · arxiv updated 2015/04/15 · openalex created_date 2022/10/04 · openalex updated_date 2026/07/31
Context. The Kepler mission has searched for planetary transits in more than two hundred thousand stars by obtaining very accurate photometric data over a long period of time. Among the thousands of detected candidates, the planetary nature of around 15% has been established or validated by different techniques. But additional data are needed to characterize the rest of the candidates and reject other possible configurations.