TESS 2 minute cadence photometry (left column), Lomb–Scargle periodogram (center column), and lightcurve phase-folded on the measured stellar rotation period (right column) for sectors 10 (top row), 36 (center row), and 63 (bottom row). The gray points in the left column panels show data points that were removed based on poor quality flags or 5σ outliers. The red curve represents the sinusoidal function that best-fits the lightcurve and represents the measured stellar rotation period. The black points in the right column represent the binned photometry.