Observations started in October 2011 and were concluded in September 2013. The first observations were carried out during ESO period P88 with the OmegaCAM STARE-mode, splitting the total exposure time into 3x480s observations with no offsets. We adopted this observing mode to obtain a constant signal-to-noise ratio (S/N) across the FOV, as in the original WINGS survey. Starting from period P89, we optimised our observing strategy, taking 5x300s exposures in DITHER-mode, with 25" and 85" offsets in horizontal and vertical direction, respectively. <P />(1 data file). <P />