  With recent developments in imaging and computer technology the amount of
available astronomical data has increased dramatically. Although most of these
data sets are not dedicated to the study of variable stars much of it can, with
the application of proper software tools, be recycled for the discovery of new
variable stars. Fits Viewer and Data Retrieval System is a new software package
that takes advantage of modern computer advances to search astronomical data
for new variable stars. More than 200 new variable stars have been found in a
data set taken with the Calvin College Rehoboth Robotic telescope using FVDRS.
One particularly interesting example is a very fast subdwarf B with a 95 minute
orbital period, the fastest currently known of the HW Vir type.
