  We present preliminary results from simulated large sky coverage (~100 square
degrees) Sunyaev-Zeldovich effect (SZE) cluster surveys using the cosmological
adaptive mesh refinement N-body/hydro code Enzo. We have generated simulated
light cones to match the resolution and sensitivity of current and future SZE
instruments. These simulations are the most advanced calculations of their
kind. The simulated sky surveys allow a direct comparison of large N-body/hydro
cosmological simulations to current and pending sky surveys. Our synthetic
surveys provide an indispensable guide for observers in the interpretation of
large area sky surveys, and will develop the tools necessary to discriminate
between models for cluster baryonic physics, and to accurately determine
cosmological parameters.
