CoRoT-7 radial velocities (Queloz+, 2009)

Queloz, D.; Bouchy, F.; Moutou, C.; Hatzes, A.; Hebrard, G.; Alonso, R.; Auvergne, M.; Baglin, A.; Barbieri, M.; Barge, P.; Benz, W.; Borde, P.; Deeg, H. J.; Deleuil, M.; Dvorak, R.; Erikson, A.; Ferraz Mello, S.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Guenther, E.; Guillot, T.; Jorda, L.; Hartmann, M.; Lammer, H.; Leger, A.; Llebaria, A.; Lovis, C.; Magain, P.; Mayor, M.; Mazeh, T.; Ollivier, M.; Patzold, M.; Pepe, F.; Rauer, H.; Rouan, D.; Schneider, J.; Segransan, D.; Udry, S.; Wuchterl, G.
Referencia bibliográfica

VizieR On-line Data Catalog: J/A+A/506/303. Originally published in: 2009A&A...506..303Q

Fecha de publicación:
10
2009
Número de autores
40
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
First, a simple pre-whitening procedure was employed to find and subsequently remove periodic signals from the complex frequency structure of the radial velocity data. The dominant frequency in the power spectrum was found at 23 days, which corresponds to the rotation period of CoRoT-7. The 0.8535 day period of CoRoT-7b planetary candidate was detected with an amplitude of 3.3m/s. (1 data file).