Doppler search for exoplanet candidates and binary stars in aCoRoTfield using a multi-fiber spectrograph

2007/03/31 by B. Loeillet, F. Bouchy, M. Deleuil +10 · 23 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Brown dwarf #Context (archaeology) #Doppler effect #Exoplanet #Geology #Giant planet #Hot Jupiter #Jupiter (rocket family) #Physics #Planet #Planetary system #Population #Space exploration #Spectral line #Spectrograph #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20077176

published in Astronomy and Astrophysics 479(3), 865-875 (EDP Sciences) · 13 pages, accepted in A&A, 2008, Volume 459, issues 2, section 13

openalex publication_date 2007/12/18 · arxiv created 2008/02/22 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.The discovery of the short-period giant exoplanet population, the so-called hot Jupiter population, and their link to brown dwarfs and low-mass stars challenges the conventional view of planet formation and evolution.

Citations

• Radius and mass of a transiting M dwarf near the hydrogen-burning limit
• An optimal extraction algorithm for CCD spectroscopy
• The WASP Project and the SuperWASP Cameras
• Catalog of Nearby Exoplanets
• Observed Properties of Exoplanets: Masses, Orbits, and Metallicities
• Doppler follow-up of OGLE transiting companions in the Galactic bulge

Cited by

• TheGaia-ESO Survey: double-, triple-, and quadruple-line spectroscopic binary candidates