  This study reports on photometric results of a search for LSB galaxies in a
0.76deg^2 field centered on the HDF-S. We present results from photometric
analysis of the derived sample galaxies and compare number densities to results
of former surveys. We used public data from the NOAO Deep Wide-Field survey and
the multi-wavelength Goddard Space Flight Center survey. The former reaches a
limiting surface brightness of mu_BW~29 magarcsec^-2 and is therefore one of
the most sensitive ground based data sets systematically analyzed for LSB
galaxies. To reduce the contamination by High Surface Brightness (HSB) galaxies
at higher redshift, mimicking LSBs due to the ''Tolman Dimming'' effect, we
placed a lower diameter limit of 10.8 arcsec and compared the colors of our
candidate galaxies with the redshift tracks of 5 ''standard'' HSB galaxy types.
We report the detection of 37 galaxies with low apparent central surface
brightness (mu_BW>=22 magarcsec^-2). Using color-color diagrams we were able to
derive a subsample of 9 LSB galaxy candidates with intrinsic central surface
brightnesses below mu_(0,BW)=22.5 magarcsec^-2 and diameters larger than the
preselected size limit of 10.8 arcsec. We selected three additional LSB
candidates due to there extreme low blue central surface brightness (mu_BW>=25
magarcsec^-2). These galaxies were only found in the larger and more sensitive
NOAO data. So finally we derived a sample of 12 LSB galaxy candidates and
therfore this survey results in a four times higher surface density than other
CCD based surveys for field galaxies before.
