  This paper is the second in a series describing the southern Galactic Disk
Survey (GDS) performed at the Universit\"atssternwarte Bochum near Cerro
Armazones in Chile. Haas et al. (2012, Paper I) presented the survey design and
a the characteristics of the observations and data. They identified ~2200
variable stars in an area of 50 square degrees with more than 50 observations
in 2011. Here we present the first complete version of the GDS covering all 268
fields with 1323 square degrees along the Galactic disk including revised data
from Paper I. The individual fields were observed up to 272 times and comprise
a maximum time span between September 2010 and May 2015. We detect a total of
64151 variable sources, which are presented in a catalog including some of
their properties and their light curves. A comparison with the International
Variable Star Index (VSX) and All Sky Automated Survey (ASAS) indicates that
56794 of these sources are previously unknown variables. Furthermore, we
present UBVr'i'z' photometry for all sources within the GDS, resulting in a new
multi-color catalog of nearly 16x10^6 sources detected in at least one filter.
Both the GDS and the near-infrared VISTA Variables in the Via Lactea survey
(VVV) complement each other in the overlap area of about 300 square degrees
enabling future comparison studies.
