CoRoT-7 radial velocities (Queloz+, 2009)

Computer Science

Scientific paper

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Stars: Dwarfs, Planets, Radial Velocities

Scientific paper

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.
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