  We present the compilation of the first 221 supernovae classified during the
Asiago Classification Program (ACP). The details of transients classification
and the preliminarily reduced spectra, in fits format, are immediately posted
on the Padova-Asiago SN group web site. The achieved performances for the first
2 years of the ACP are analysed, showing that half of all our classifications
were made within 5 days from transient detection. The distribution of the
supernova types of this sample resembles the distribution of the general list
of all the supernovae listed in the Asiago SN catalog (ASNC, Barbon et al.
1999). Finally, we use our sub-sample of 78 core-collapse supernovae, for which
we retrieve the host-galaxy morphology and r-band absolute magnitudes, to study
the observed subtype distribution in dwarf compared to giant galaxies. This
ongoing program will give its contribution to the classification of the large
number of transients that will be soon delivered by the Gaia mission.
