Order-per-order weight profiles of intrinsic stellar spectra near the second (blue) and third (red) transit contacts of WASP-76 in epoch 1, as a function of wavelength in the surface rest frame. Besides the contributions highlighted in Fig. 19, we note the impact of masked planetary ranges (which redshift over the transit as the planet orbits faster than the star rotates) and disk-integrated stellar lines (which blueshift over the transit as the planet first occults the stellar hemisphere rotating toward, and then away, from the observer; see inset).