We have searched data for gravitational-wave signals from white dwarf binaries 
in the frequency band from 0.16mHz to 12 mHz. We have detected and estimated 
parameters of 14838 signals. Our algorithm was as follows. We have divided data 
in narrow bands of 0.1mHz. In each band we have searched for the strongest signal.
We have estimated its parameters, reconstructed the signal and removed
it from the time series. Then we went to the next strongest signal and
iterated untill a certain threshold signal-to-noise ratio.
Above the frequency of 3mHz we have included the frequency derivative parameter.
Below the frequency of 3mHz we had SNR threshold equal to 9 and above 3 mHz
the threshold equal to 6.
The data analysis method was matched filtering using the F-statistic for
A and E componenets. We have used analytic filters in the adiabatic approximation.