The main goal of the WFI Pilot Survey (PS) was to complement
with B,V observations the area covered by the EIS-WIDE I-band survey
and to be a pathfinder for future public imaging surveys programs to be carried out
with the WFI@NTT. With this spirit, the WFI Pilot Survey was endoarsed by the
A total area of about 14 square degrees were
In addition, BVI data for
selected Stellar Fields have been obtained as a test case for
the Pre-FLAMES Survey.
Observations have been performed during periods ESO.62-ESO.64 . The WFI Pilot
Survey was completed on September 1999.