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[Abridged] To effectively investigate galaxy formation and evolution, it isof paramount importance to exploit homogeneous data for large samples ofgalaxies in different environments. The WINGS (WIde-field Nearby Galaxy-clusterSurvey) project aim is to evaluate physical properties of galaxies in acomplete sample of low redshift clusters to be used as reference sample forevolutionary studies. The WINGS survey is still ongoing and the originaldataset will soon be enlarged with new observations. This paper presents theentire collection of WINGS measurements obtained so far. We decided to make useof the Virtual Observatory (VO) tools to share the WINGS database (that will beregularly updated) with the community. In the database each object has oneunique identification (WINGSID). Each subset of estimated properties isaccessible using a simple cone search (including wide-field images). We providethe scientific community the entire set of wide-field images. Furthermore, thepublished database contains photometry of 759,024 objects and surfacebrightness analysis for 42,275 and 41,463 galaxies in the V and B band,respectively. The completeness depends on the image quality, and on the clusterredshift, reaching on average 90% at V<= 21.7. Near infrared photometriccatalogs for 26 (in K) and 19 (in J) clusters are part of the database and thenumber of sources is 962,344 in K and 628,813 in J. Here again the completenessdepends on the data quality, but it is on average higher than 90% for J<=20.5and K<=19.4. The IR subsample with a Sersic fit comprises 71,687 objects. Amorphological classification is available for 39,923 galaxies. We publishspectroscopic data, including 6,132 redshifts, 5,299 star formation historiesand 4,381 equivalent widths. Finally, a calculation of local density ispresented and implemented in the VO catalogs for 66,164 galaxies.

WINGS Data Release: a database of galaxies in nearby clusters