  We study a small sample of z=0.1-0.6 core-collapse supernova (CCSN) host
galaxies. Continuum observations at 250GHz have been performed with MAMBO at
the IRAM-30m telescope. None of these sources has been detected and the
error-weighted mean flux is 0.25+/-0.32 mJy. Upper limits on their dust masses
are derived and the corresponding sample mean corresponds to 1.4 +/- 2.2 x 10^8
Msol. These results are comparable with previous submillimetre observations of
SN-Ia hosts performed by Farrah et al. and by Clements et al. We conclude that
CCSN hosts are not extreme at millimetre wavelengths, and as confirmed with the
optical luminosities of a subset of our sample, they are typical of the local
galaxy population.
