Fig. 1.
Top: HQ Tau’s detrended Kepler K2 light curve. Low frequency variations have been removed from the original light curve shown in Fig. 2. The spike appearing at J.D. 2 457 890.0 is presumably an instrumental defect. Middle: HQ Tau’s light curve folded in phase with P = 2.424 d. The origin of phase is taken as JD 2 457 823.81 to correspond to the epoch of maximum brightness. Bottom: lomb-Scargle periodogram obtained from HQ Tau’s Kepler K2 light curve.
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