TESS simple aperture photometry light curve of WASP-167 (top row, grey dots) from Sectors 10 (left), 37 (middle), and 64 (right). The masked, detrended, and centroid-corrected LC is shown in black. The pulsation model, constructed from the 16 highest amplitude sinusoidal curves, is shown in the second row as a solid magenta line. The blue dots in the third row represent the LC when these 16 highest amplitude pulsations have been removed, while the best-fit combination of time-correlated noise and phase curve models are shown in red. The residuals, along with their root mean square error (RMSE) are shown in the bottom row.