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This is an introduction to the tabulated data base of stellar matterproperties calculated within the framework of the Statistical Model forSupernova Matter (SMSM). The tables present thermodynamical characteristics andnuclear abundances for 31 values of baryon density (10$^{-8}<\rho/\rho_0<$0.32,$\rho_0$=0.15 fm$^{-3}$ is the normal nuclear matter density), 35 values oftemperature ($0.2<T<25$ MeV) and 28 values of electron-to-baryon ratio($0.02<Y_e<0.56$). The properties of stellar matter in $\beta$-equilibrium arealso considered. The main ingredients of the SMSM are briefly outlined, and thedata structure and content of the tables are explained.

Tabulated equation of state for supernova matter including full nuclear ensemble