  The SOXS spectrograph, designed for the ESO NTT telescope, operates in both
the optical (UV-VIS: 350-850 nm) and NIR (800-2000 nm) bands. This article
provides an overview of the final tests conducted on the UV-VIS camera system
using a telescope simulator. It details the system's performance evaluation,
including key metrics such as gain, readout noise, and linearity, and
highlights the advancements made in the upgraded acquisition system. The
testing process, conducted in the Padua laboratory, involved comprehensive
simulations of the telescope environment to ensure the results closely resemble
those expected at the ESO-NTT telescope. The successful completion of these
tests confirms the system's readiness for deployment to Chile, where it will be
installed on the NTT telescope, marking a significant milestone in the SOXS
project.
