Fig. B.3.
Amplitude spectra of the BRITE-Constellation data obtained in 2017 with BAb only: Top panel: amplitude spectrum of the original data with F1 identified, middle panel: amplitude spectrum after pre-whitening F1, and bottom panel: residuals after pre-whitening with the significant frequencies. We note that the noise of the 2017 BAb data is significantly higher than for all the other combined data sets, hence F3 remains hidden in the noise.
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