  Time-series photometry of the CoRoT field SRc02 was obtained by the Berlin
Exoplanet Search Telescope II (BEST II) in 2009. The main aim was the ground
based follow-up of the CoRoT field in order to detect variable stars with
better spatial resolution than what can be achieved with the CoRoT space
telescope. A total of 1,846 variable stars were detected, of which only 30 have
been previously known. For nine eclipsing binaries the stellar parameters were
determined by modeling their light curve.
