Fig. 4
Frequency analysis of the Be star CoRoT 102672979 (star No 5) observed in the LRA1 run. Panel a: rectified light curve; panel b: rectified light curve corrected from the shape of the outburst. Panel c: DFT of the corrected light curve shown in (b); we note the low number of frequencies in group 1 ~ 0 c d−1; panel d: DFT zoomed on the second frequency group located at 0.8 c d−1; and panel e: DFT zoomed on the third frequency group located at 1.6 c d−1.
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