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The WIde-field Nearby Galaxy clusters Survey (WINGS) is a project whoseprimary goal is to study the galaxy populations in clusters in the localuniverse (z<0.07) and of the influence of environment on their stellarpopulations. This survey has provided the astronomical community with a highquality set of photometric and spectroscopic data for 77 and 48 nearby galaxyclusters, respectively. In this paper we present the catalog containing theproperties of galaxies observed by the WINGS SPEctroscopic (WINGS-SPE) survey,which were derived using stellar populations synthesis modelling approach. Wealso check the consistency of our results with other data in the literature.Using a spectrophotometric model that reproduces the main features of observedspectra by summing the theoretical spectra of simple stellar populations ofdifferent ages, we derive the stellar masses, star formation histories, averageage and dust attenuation of galaxies in our sample. ~5300 spectra were analyzedwith spectrophotometric techniques, and this allowed us to derive the starformation history, stellar masses and ages, and extinction for the WINGSspectroscopic sample that we present in this paper. The comparison with thetotal mass values of the same galaxies derived by other authors based on SDSSdata, confirms the reliability of the adopted methods and data.

WINGS-SPE II: A catalog of stellar ages and star formation histories, stellar masses and dust extinction values for local clusters galaxies