  In February 2014, the SHARK-VIS (System for High contrast And coronography
from R to K at VISual bands) Forerunner, a high contrast experimental imager
operating at visible wavelengths, was installed at LBT (Large Binocular
Telescope). Here we report on the first results obtained by recent on-sky
tests. These results show the extremely good performance of the LBT ExAO
(Extreme Adaptive Optics) system at visible wavelengths, both in terms of
spatial resolution and contrast achieved. Similarly to what was done by (Amara
et al. 2012), we used the SHARK-VIS Forerunner data to quantitatively assess
the contrast enhancement. This is done by injecting several different synthetic
faint objects in the acquired data and applying the ADI (angular differential
imaging) technique. A contrast of the order of $5 \times 10^{-5}$ is obtained
at 630 nm for angular separations from the star larger than 100 mas. These
results are discussed in light of the future development of SHARK-VIS and
compared to those obtained by other high contrast imagers operating at similar
wavelengths.
