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Radial velocity follow-up for confirmation and characterization of transiting exoplanets

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arxiv 0902.3520 v1 pith:5I4FGNYB submitted 2009-02-20 astro-ph.EP

F. Bouchy , C. Moutou , D. Queloz , the CoRoT Exoplanet Science Team This is my paper · ORCID
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keywords follow-uptransitingradialvelocitycandidatescharacterizationsomestrategy
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Radial Velocity follow-up is essential to establish or exclude the planetary nature of a transiting companion as well as to accurately determine its mass. Here we present some elements of an efficient Doppler follow-up strategy, based on high-resolution spectroscopy, devoted to the characterization of transiting candidates. Some aspects and results of the radial velocity follow-up of the CoRoT space mission are presented in order to illustrate the strategy used to deal with the zoo of transiting candidates.

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Cited by 1 Pith paper

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  1. Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned

    astro-ph.EP 2026-07 conditional novelty 6.0 of 10

    Warm sub-Saturns around single cool stars are predominantly aligned whereas hot sub-Saturns are frequently misaligned (3.2σ), a separation-dependent transition the authors attribute to high-eccentricity migration.

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