  Hot Jupiters, particularly those with temperature higher than 2000 K are the
best sample of planets that allow in-depth characterization of their
atmospheres. We present here a thermal emission study of the ultra hot Jupiter
WASP-103 b observed in two secondary eclipses with CFHT/WIRCam in J and Ks
bands. By means of high precision differential photometry, we determine eclipse
depths in J and Ks to an accuracy of 220 and 270 ppm, which are combined with
the published HST/WFC3 and Spitzer data to retrieve a joint constraints on the
properties of WASP-103 b dayside atmosphere. We find that the atmosphere is
best fit with a thermal inversion layer included. The equilibrium chemistry
retrieval indicates an enhanced C/O (1.35$^{+0.14}_{-0.17}$) and a super
metallicity with [Fe/H]$=2.19^{+0.51}_{-0.63}$ composition. Given the
near-solar metallicity of WASP-103 of [Fe/H]=0.06, this planet seems to be
$\sim$100 more abundant than its host star. The free chemistry retrieval
analysis yields a large abundance of FeH, H$^{-}$, CO$_2$ and CH$_4$.
Additional data of better accuracy from future observations of JWST should
provide better constraint of the atmospheric properties of WASP-103b.
