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\subsection{Reduction}  The Herschel SPIRE FTS data were obtained over xxx-xxx and reduced as explained indetail in  Pellegrini et al., in prep. As a summary, we applied the calibration pipeline up to a certain point. However, corrections in between those of an extended and point source were required for all but three galaxies (NGC 1266, NGC 1377 and NGC 3351, hereafter `point-source galaxies'). We made such corrections based upon the spatial distribution of the FIR emission in the SPIRE 250 micron maps, assuming the dust and gas will to follow each other, to first order. \subsection{[CI] maps and morphologies}