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The Capodimonte Deep Field (OACDF) is a multi-colour imaging survey on two0.5x0.5 square degree fields performed in the BVRI bands and in six medium-bandfilters (700 - 900 nm) with the Wide Field Imager (WFI) at the ESO 2.2 mtelescope at La Silla, Chile. In this contribution the adopted strategies forthe OACDF data reduction are discussed. Preliminary scientific results of thesurvey are also presented.Comment: 12 pages, 10 figures, to be presented at "Astronomical Telescopes &  Instrumentation", SPIE 2002; corrected authors lis

Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field