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20032008
most citedTW Hydrae: evidence of stellar spots instead of a Hot Jupiter

242 citations · 699 across the 5 of their papers we have counts for

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astro-ph2008242 cited

TW Hydrae: evidence of stellar spots instead of a Hot Jupiter

N. Huelamo, P. Figueira, X. Bonfils +12

TW Hydrae shows significant radial-velocity variations in the optical regime. They have been attributed to a 10 Jupiter Mass planet orbiting the star at 0.04 AU. In this work, we h…

astro-ph200865 cited

A near-infrared interferometric survey of debris disc stars. II. CHARA/FLUOR observations of six early-type dwarfs

O. Absil, E. Di Folco, A. Merand +15

High-precision interferometric observations of six early-type main sequence stars known to harbour cold debris discs have been obtained in the near-infrared K band with the FLUOR i…

astro-ph200785 cited

A near-infrared interferometric survey of debris disk stars. I. Probing the hot dust content around epsilon Eridani and tau Ceti with CHARA/FLUOR

E. Di Folco, O. Absil, J. -C. Augereau +11

We probed the first 3AU around tau Ceti and epsilon Eridani with the CHARA array (Mt Wilson, USA) in order to gauge the 2micron excess flux emanating from possible hot dust grains…

astro-ph2006139 cited

Circumstellar material in the Vega inner system revealed by CHARA/FLUOR

O. Absil, E. di Folco, A. Merand +11

Only a handful of debris disks have been imaged up to now. Due to the need for high dynamic range and high angular resolution, very little is known about the inner planetary region…

astro-ph2006168 cited

First Results from the CHARA Array VII: Long-Baseline Interferometric Measurements of Vega Consistent with a Pole-On, Rapidly Rotating Star

J. P. Aufdenberg, A. Merand, V. Coude du Foresto +10

We have obtained high-precision interferometric measurements of Vega with the CHARA Array and FLUOR beam combiner in the K' band at projected baselines between 103m and 273m. The m…

astro-ph2004

The angular size of dwarf stars and subgiants - Surface brightness relations calibrated by interferometry

P. Kervella, F. Thevenin, E. Di Folco +1

The availability of a number of new interferometric measurements of Main Sequence and subgiant stars makes it possible to calibrate the surface brightness relations of these stars…