PACS spectrum of the nebula around AG Car, integrated over the 25 spaxels. Indicated are the lines [Oi], [Nii], and [Cii]. Below 55 μm the shape of the continuum results from a spectral response function correction that has not yet been perfected. Above 190 μm the shape results from a light leak from the second diffraction order of the grating in the first one. The different observing bands are indicated with different colors. We note that the spectral resolution depends on the waveband.