  In this paper, we present a set of photometric observations in 15 colors of
stars in the Landolt covered by the system range from 300 nm to 1000 nm. Visual
magnitudes of the stars being studied in the field are from 10th to 20th mag.
The observational methodology and the data reduction procedures are described.
The relationships between the BATC intermediate-band system and the Landolt
UBVRI broad band system are obtained. A catalogue of the photometry has been
produced which contains the SEDs of 3613 stars. The electronic form of this
catalogue can be accessed at the CDS via anonymous ftp to cdsarc.u-strasbg.fr.
