Cylindrical power spectra for the remaining full-sky simulations that were not shown in Fig. 7. For each location, the two rows correspond to the celestial pole (top) and zenith transit (bottom) phase center declinations. In the lowermost row, for the simulations centered at LST = 9h, 13h, and 17h, the phase center is below the horizon for part of the observation, and hence the visibilities are not predicted. The full synthesis line is not shown in this case since it is vertical (from Eq. (15)).