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20072025
most citedSOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

273 citations · 3.4k across the 67 of their papers we have counts for

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Showing 2012Show all

5 papers · 1 filter

astro-ph.IM2012★ 143 cited

SOPHIE+: First results of an octagonal-section fiber for high-precision radial velocity measurements

F. Bouchy, R. F. Diaz, G. Hébrard +5

High-precision spectrographs play a key role in exoplanet searches and Doppler asteroseismology using the radial velocity technique. The 1 m/s level of precision requires very high…

astro-ph.EP2012★ 41 cited

SOPHIE velocimetry of Kepler transit candidates VI. An additional companion in the KOI-13 system

A. Santerne, C. Moutou, S. C. C. Barros +7

We report the discovery of a new stellar companion in the KOI-13 system. KOI-13 is composed by two fast-rotating A-type stars of similar magnitude. One of these two stars hosts a t…

astro-ph.EP2012★ 183 cited

SOPHIE velocimetry of Kepler transit candidates VII. A false-positive rate of 35% for Kepler close-in giant exoplanet candidates

A. Santerne, R. F. Díaz, C. Moutou +6

The false-positive probability (FPP) of Kepler transiting candidates is a key value for statistical studies of candidate properties. A previous investigation of the stellar populat…

astro-ph.EP2012★ 60 cited

The SOPHIE search for northern extrasolar planets. V. Follow-up of ELODIE candidates: Jupiter-analogs around Sun-like stars

I. Boisse, F. Pepe, C. Perrier +21

We present radial-velocity measurements obtained in a programs underway to search for extrasolar planets with the spectrograph SOPHIE at the 1.93-m telescope of the Haute-Provence…

astro-ph.EP2012★ 33 cited

Transiting exoplanets from the CoRoT space mission XXI. CoRoT-19b: A low density planet orbiting an old inactive F9V-star

E. W. Guenther, R. F. Diaz, J. -C. Gazzano +51

Observations of transiting extrasolar planets are of key importance to our understanding of planets because their mass, radius, and mass density can be determined. The CoRoT space…