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The VST Early-type GAlaxy Survey (VEGAS) is a deep, multi-band (u, g, r, i)imaging survey, carried out with the 2.6-metre VLT Survey Telescope (VST) atESO's Paranal Observatory in Chile. VEGAS combines the wide (1-square-degree)OmegaCAM imager and long integration times, together with a specially designedobserving strategy. It has proven to be a gold mine for studies of features atvery low surface brightness, down to levels of mu_g~27-30 magnitudesarcsec^(-2), over 5-8 magnitudes fainter than the dark sky at Paranal. In thisarticle we highlight the main science results obtained with VEGAS observationsof galaxies across different environments, from dense clusters of galaxies tounexplored poor groups and in the field.

The VST Early-type GAlaxy Survey: Exploring the Outskirts and Intra-cluster Regions of Galaxies in the Low-surface-brightness Regime