The GAPS programme with HARPS-N at TNG

2013/04/09 by E. Covino, M. Esposito, M. Barbieri +76
Physics and Astronomy · #Aerospace engineering #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Emission spectrum #Equivalent width #Geometry #Light curve #Line (geometry) #Orbit (dynamics) #Physics #Planet #Planetary system #Radial velocity #Spectral energy distribution #Spectral line #Star (game theory) #Stars #Stellar, planetary, and galactic studies #Transit (satellite) #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201321298

12 pages, 8 figures

arxiv created 2013/04/09 · openalex publication_date 2013/04/12 · arxiv updated 2015/06/15 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/01

Abstract

Context. Our understanding of the formation and evolution of planetary systems is still fragmentary because most of the current data provide limited information about the orbital structure and dynamics of these systems. The knowledge of the orbital properties for a variety of systems and at different ages yields information on planet migration and on star-planet tidal interaction mechanisms.

Citations

• TWO “b”s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER
• A Subspace, Interior, and Conjugate Gradient Method for Large-Scale Bound-Constrained Minimization Problems
• Tidal Dissipation in Rotating Solar‐Type Stars
• Homogeneous studies of transiting extrasolar planets – I. Light-curve analyses
• Effective temperature scale and bolometric corrections from 2MASS photometry
• Hot Jupiters and the evolution of stellar angular momentum
• Improved Age Estimation for Solar‐Type Dwarfs Using Activity‐Rotation Diagnostics
• A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)
• OBSERVATIONAL EVIDENCE FOR TIDAL DESTRUCTION OF EXOPLANETS
• tempo2, a new pulsar-timing package - I. An overview
• Elemental abundances of low-mass stars in nearby young associations:AB Doradus, Carina Near and Ursa Major
• The NextGen Model Atmosphere Grid for \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape 3000≤ T_eff ≤ 10,000 \enddocument K
• Properties of planets in binary systems