  We present precise V and Ks-band transit photometry for the planetary host
star OGLE-TR-113. Using the Ks-band photometry, we confirm the dwarf nature of
OGLE-TR-113, and obtain new estimates for its effective temperature, distance
and reddening. We employ the V-band photometry to obtain planetary and orbit
parameters from the transit fit, a= (0.0232 \pm 0.0038) AU, orbital period P=
(1.4324752 \pm 0.0000015) days, i= 86.7 - 90, R_p= (1.09 \pm 0.09) R_J. These
values are in excellent agreement with previous works. Assuming a mass M_p=
(1.32 \pm 0.19) M_J for the planet we obtain its mean density \rho= (1.26 \pm
0.50) g cm^{-3}, also in agreement with previous works. The transit observed in
the Ks-band has a larger scatter and we find its amplitude to be consistent
with that in the V-band. In this way, we find an independent confirmation of
the planetary nature of OGLE-TR-113b.
