  In this paper we present CCD spectrophotometry of the star clusters that were
detected by Chandar, Bianchi, & Ford in the nearby spiral galaxy M33, using the
images obtained with the Beijing Astronomical Observatory 60/90 cm Schmidt
Telescope in 13 intermediate-band filters from 3800 to 10000{\AA}. The
observations cover the whole area of M33 with a total integration of 32.75
hours from September 23, 1995 to August 28, 2000. This provides a multi-color
map of M33 in pixels of $1.7'' \times 1.7''$. By aperture photometry, we obtain
the spetral energy distributions (SEDs) of these star clusters. Using
theoretical stellar population synthesis models, we also obtain the
distributions of age and metallicity of of these star clusters. These clusters
formed continuously from $\sim 3\times10^6$ -- $10^{10}$ years, and have a
large span of metallicity from ${\rm {Z}=0.0004}$ to ${\rm {Z}=0.05}$.
