  NASA's Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey
mission designed to find transiting exoplanets orbiting nearby bright stars. It
has identified more than 329 transiting exoplanets, and almost 6,000 candidates
remain unvalidated. In this manuscript, we discuss the findings from the
ongoing VaTEST (Validation of Transiting Exoplanets using Statistical Tools)
project, which aims to validate new exoplanets for further characterization. We
validated 11 new exoplanets by examining the light curves of 24 candidates
using the LATTE and TESS-Plot tools and computing the False Positive
Probabilities using the statistical validation tool TRICERATOPS. These include
planets suitable for atmospheric characterization using transmission
spectroscopy (TOI-2194b), emission spectroscopy (TOI-3082b and TOI-5704b) and
for both transmission and emission spectroscopy (TOI-672b, TOI- 1694b, and
TOI-2443b); One super-Earth (TOI-2194b) orbiting a bright (V = 8.42 mag),
metal-poor ([Fe/H] = -0.3720 $\pm$ 0.1) star; one short-period Neptune-like
planet (TOI-5704) in the Hot Neptune Desert. In total, we validated 1
super-Earth, 7 sub-Neptunes, 1 Neptune-like, and 2 sub-Saturn or
super-Neptune-like exoplanets. Additionally, we identify five likely planet
candidates (TOI-323, TOI- 1180, TOI-2200, TOI-2408 and TOI-3913) which can be
further studied to establish their planetary nature.
