  We discuss the progress of the SCUBA Local Universe Galaxy Survey (SLUGS),
the first large, statistical sub-mm survey of the local universe. Since our
original survey of a sample of 104 IRAS-selected galaxies we have recently
completed a sample of 78 Optically-Selected galaxies. Since SCUBA is sensitive
to the large proportion of dust too cold to be detected by IRAS the addition of
this optically-selected sample allows us for the first time to determine the
amount of cold dust in galaxies of different Hubble types. We detect 6
ellipticals in the sample and find them to have dust masses in excess of 10^7
solar masses. We derive local sub-mm luminosity functions, both directly for
the two samples, and by extrapolation from the IRAS PSCz, and find excellent
agreement.
