  Observations of diffuse starlight in the outskirts of galaxies are thought to
be a fundamental source of constraints on the cosmological context of galaxy
assembly in the $\Lambda$CDM model. Such observations are not trivial because
of the extreme faintness of such regions. In this work, we investigate the
photometric properties of six massive early type galaxies (ETGs) in the VEGAS
sample (NGC 1399, NGC 3923, NGC 4365, NGC 4472, NGC 5044, and NGC 5846) out to
extremely low surface brightness levels, with the goal of characterizing the
global structure of their light profiles for comparison to state-of-the-art
galaxy formation models. We carry out deep and detailed photometric mapping of
our ETG sample taking advantage of deep imaging with VST/OmegaCAM in the g and
i bands. By fitting the light profiles, and comparing the results to
simulations of elliptical galaxy assembly, we identify signatures of a
transition between "relaxed" and "unrelaxed" accreted components and can
constrain the balance between in situ and accreted stars. The very good
agreement of our results with predictions from theoretical simulations
demonstrates that the full VEGAS sample of $\sim 100$ ETGs will allow us to use
the distribution of diffuse light as a robust statistical probe of the
hierarchical assembly of massive galaxies.
