Radial velocity follow-up of CoRoT transiting exoplanets

被引：7
|
作者：
Santerne, A. [1 ,2 ]
Endl, M. [3 ]
Hatzes, A. [4 ]
Bouchy, F. [2 ,5 ]
Moutou, C. [1 ]
Deleuil, M. [1 ]
机构：
[1] CNRS, Lab Astrophys Marseille, Marseille, France
[2] Univ Aix Marseille 1, CNRS, Observ Haute Provence, Marseille, France
[3] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA
[4] Thuringer Landessternwarte, D-07778 Tautenburg, Germany
[5] Inst Astrophys Paris, F-75014 Paris, France
来源：
DETECTION AND DYNAMICS OF TRANSITING EXOPLANETS | 2011年 / 11卷
关键词：
SPACE MISSION;
D O I：
10.1051/epjconf/20111102001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on the results from the radial-velocity follow-up program performed to establish the planetary nature and to characterize the transiting candidates discovered by the space mission CoRoT. We use the SOPHIE at OHP, HARPS at ESO and the HIRES at Keck spectrographs to collect spectra and high-precision radial velocity (RV) measurements for several dozens different candidates from CoRoT. We have measured the Rossiter-McLaughlin effect of several confirmed planets, especially CoRoT-1b which revealed that it is another highly inclined system. Such high-precision RV data are necessary for the discovery of new transiting planets. Furthermore, several low mass planet candidates have emerged from our Keck and HARPS data.
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页数：9
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