Fig. 7.
Zoom around F13 (left side, seen alongside with F14 in the 2015 data to the right of F13) and F11 (right side) into the original amplitude spectra of the BRITE red-filter data obtained in 2015 (top), 2016/2017 (middle), and 2017/2018 (bottom). The peak next to F13 in the bottom left panel showing the 2017/18 data is an alias frequency to F3 with the orbital frequency of BHr (i.e., 14.83053 d−1) that only appears quite close to the location of F14, which itself is not found in the 2017/18 data.
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