Results from joint fitting WIRC night 1 (blue), WIRC night 2 (red), and TESS (gray) data. Panel (a) shows the phase-folded light curves for all three time series. Individual points and their uncertainties are shown with small markers, and Palomar/WIRC data binned to 10 minute intervals are shown with larger markers. Best-fit light-curve models are shown as solid lines. Panels (b), (c), and (d) show the residuals for the WIRC night 1, WIRC night 2, and TESS time series, respectively.