Fig. 8
Frequency analysis of the Be star CoRoT 102766835 (star No 14) observed first in the IR1 (in green), then in the LRA1 (in blue). Panel a: rectified light curve (IR1); panel b: rectified light curve (LRA1); panel c: DFT of the rectified light curve in each run (green dashed line for the IR1 and blue full line for the LRA1); panel d: DFT zoomed in each run on the second frequency group located at 0.85 c d−1; and panel e: DFT zoomed in each run on the third and fourth frequency groups located at 1.7 c d−1 and 2.5 c d−1.
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