Two hundred and twenty-five raw spectra obtained with the PACS 5 × 5 detector array on all of the 3 × 3 raster map positions on Saturn at 66.44 μm. The 25 spectra recorded by the detector array are plotted for each of the 9 raster map positions. The H₂O line is detected in all spectra corresponding to pointings on the planetary disk or close to the planetary limb. Spectra without an H₂O line correspond to pointings far off the planetary limb. Before fitting the lines with a Gaussian to compute their area,a polynomial baseline was removed from these spectra. The line peak S/N around the limb is ~ 15–45.