  Our goal is to investigate the spiral structure of the Northern Galactic
plane using as tracers the classical Be stars detected by INT Photometric
H$\alpha$ Survey (IPHAS). IPHAS scans the $29^o<l<+215^o, -5^o<b<+5^o$ region
in the $r$, $i$ and H$\alpha$ bands. Spectroscopic follow up has been done for
the bright H$\alpha$ emitters. We have developed an automatic procedure for
spectral analysis, based on the BCD spectrophotometric system. In this paper we
present a cataloque of 1135 Classical Be stars, for which we have determined
spectral types, astrophysical parameters and distances. From these results we
make a first attempt to map the structure of the Galactic disk in the
anticenter direction.
