  It is well known that N-body simulations of ultralight bosons show the
formation of a solitonic dark matter core in the innermost part of the halo.
The scale length of such a soliton depends on the inverse of the mass of the
boson. On the other hand, the orbital motion of stars in the Galactic Center
depends on the distribution of matter whether be it baryonic or dark, providing
an excellent probe for the gravitational field of the region. In this Letter we
propose the S-stars in the Galactic Center as a new observational tool,
complementary to other astrophysical systems, to narrow down the range of
allowed values for an ultralight dark matter candidate boson mass. We built
mock catalogs mirroring the forthcoming astrometric and spectroscopic
observations of S2, and we used a MCMC analysis to predict the accuracy down to
which the mass of an ultralight boson may be bounded, and we showed that, once
complementary constraints are considered, this analysis will help to restrict
the allowed range of the boson mass. Our analysis forecasts the bound on the
mass of an ultralight boson to be $< 10^{-19}$ eV at the 95% of confidence
level.
