  We have started a large survey for double degenerate (DD) binaries as
potential progenitors of type Ia supernovae with the UVES spectrograph at the
ESO VLT (ESO SN Ia Progenitor surveY - SPY). About 400 white dwarfs were
checked for radial velocity variations during the first 15 months of this
project, twice the number of white dwarfs investigated during the last 20
years. We give an overview of the SPY project and present first results Fifty
four new DDs have been discovered, seven of them double lined (only 18 and 6
objects of these groups were known before, respectively). The final sample is
expected to contain 150 to 200 DDs. Eight new pre-cataclysmic binaries were
also detected. SPY is the first DD survey which encompasses also non-DA white
dwarfs. SPY produces an immense, unique sample of very high resolution white
dwarf spectra, which provides a lot of spin-off opportunities. We describe our
projects to exploit the SPY sample for the determination of basic parameters,
kinematics, and rotational velocities of white dwarfs. A catalogue with a first
subset of our white dwarf data has already been published by Koester et al.
2001.
