Frequency spectra of the red 2016 BRITE observations before (top) and after (bottom) mJD 600 when a series of brightenings began (see Fig. 1). Power is given in arbitrary units. The arrows have the same meaning as in Fig. 7, and the full-season error curve (arbitrarily scaled) from Fig. 7 is also shown. In the top panel, frequency groups g1 (1.0–1.7 c/d)and g2 (2.2–3.0 c/d) are well separated.
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