Fig. 6
Frequency analysis of the Be star CoRoT 102719279 (star No 9) observed first in the IR1 (in green), then in the LRA1 (in blue). Panel a: rectified light curve (IR1); panel b: rectified light curve (IR1) corrected from the shape of the outburst; panel c: rectified light curve (LRA1); panel d: rectified light curve (LRA1) corrected from the shape of the strong outburst; panel e: DFT is shown of the corrected light curves shown in (b) and (d) for the IR1 (green dashed line) and the LRA1 (blue full line), respectively; panel f: DFT zoomed in each run on the second frequency group located at 1.1 c d−1; and panel g: DFT zoomed in each run on the third frequency group located at 2.3 c d−1.
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