The galaxies UGCA 86, UGCA 92, UGCA 105, NGC 1569, and Cas 1 were observed
in February 5-7, 1995 at the Nordic 2.5-meter telescope in the V and I
bands of the Kron-Cousins system. The observations were carried out with a
TK 1024A CCD chip having 1024 by 1024 pixels each 24 microns in size. It
provided a 
field of view with the resolution of
per pixel. The CCD quantum efficiency is about 70% in each of
the bands, and the read-out noise is 
. The frames of the galaxies
were obtained under quite good photometric conditions with a seeing of FMHM
. Table 1 (click here) describes the exposures.
After subtracting dark frame, flat-fielding and cleaning of cosmic ray events the photometric processing of the frames was performed with DAOPHOT and ALLSTAR packages (Stetson 1987). Equatorial photometric standards from Landolt (1992) were observed in order to transform instrumental magnitudes into the standard V and I system. According to our estimate the total error in the zero-point does not exceed 0.05 mag for any of the galaxies.