The linear optical properties of Cu2ZnSnS4 bulk poly-crystals have been investigated using spectroscopic ellipsometry in the range 1.2-4.6 eV at room temperature. The characteristic features identified in the optical spectra are explained by using the Adachi analytical model for the interband transitions at the corresponding critical points in the Brillouin zone (BZ). The experimental data have been modeled over the entire spectral range taking into account the lowest E0 transition near the fundamental absorption edge, and E1A and E1B higher energy interband transitions. In addition, the spectral dependences of the refractive index, extinction coefficient, absorption coefficient, and normal-incidence reflectivity values have been determined and are provided since they are essential data for the design of Cu2ZnSnS4 based optoelectronic devices. In the span of the last decade, much progress has been made in the kesterite based Cu2ZnSnS4 (CZTS) thin film solar cells. This is because kesterites show excellent properties as absorber materials such as an optimal band gap of ~ 1.5 eV 1-3 which can be tuned by adjusting anion and cation compositions 4,5 and a high optical absorption coefficient 6,7 over ~10 4 cm-1. Moreover, the kesterites are constituted by low-cost elements with low toxicity and abundant in the Earth's crust, which allows avoiding the use of critical raw materials.